National Library of Energy BETA

Sample records for matter ppm parts

  1. PPM Atlantic Renewable Formerly Atlantic Renewable Energy Corp...

    Open Energy Info (EERE)

    PPM Atlantic Renewable Formerly Atlantic Renewable Energy Corp Jump to: navigation, search Name: PPM Atlantic Renewable (Formerly Atlantic Renewable Energy Corp) Place: Virginia...

  2. Simulating Rayleigh-Taylor (RT) instability using PPM hydrodynamics @scale on Roadrunner (u)

    SciTech Connect (OSTI)

    Woodward, Paul R; Dimonte, Guy; Rockefeller, Gabriel M; Fryer, Christopher L; Dimonte, Guy; Dai, W; Kares, R. J.

    2011-01-05

    The effect of initial conditions on the self-similar growth of the RT instability is investigated using a hydrodynamics code based on the piecewise-parabolic-method (PPM). The PPM code was converted to the hybrid architecture of Roadrunner in order to perform the simulations at extremely high speed and spatial resolution. This paper describes the code conversion to the Cell processor, the scaling studies to 12 CU's on Roadrunner and results on the dependence of the RT growth rate on initial conditions. The relevance of the Roadrunner implementation of this PPM code to other existing and anticipated computer architectures is also discussed.

  3. Respiratory responses of vigorously exercising children to 0. 12 ppm ozone exposure

    SciTech Connect (OSTI)

    McDonnell, W.F. 3d.; Chapman, R.S.; Leigh, M.W.; Strope, G.L.; Collier, A.M.

    1985-10-01

    Changes in respiratory function have been suggested for children exposed to less than 0.12 ppm ozone (O3) while engaged in normal activities. Because the results of these studies have been confounded by other variables, such as temperature or the presence of other pollutants or have been questioned as to the adequacy of exposure measurements, the authors determined the acute response of children exposed to 0.12 ppm O3 in a controlled chamber environment. Twenty-three white males 8 to 11 yr of age were exposed once to clean air and once to 0.12 ppm O3 in random order. Exposures were for 2.5 h and included 2 h of intermittent heavy exercise. Measures of forced expiratory volume in one second (FEV1) and the symptom cough were determined prior to and after each exposure. A significant decline in FEV1 was found after the O3 exposure compared to the air exposure, and it appeared to persist for 16 to 20 h. No significant increase in cough was found due to O3 exposure. Forced vital capacity, specific airways resistance, respiratory frequency, tidal volume, and other symptoms were measured in a secondary exploratory analysis of this study.

  4. Pulmonary function and symptom responses after 6. 6-hour exposure to 0. 12 ppm ozone with moderate exercise

    SciTech Connect (OSTI)

    Folinsbee, L.J.; McDonnell, W.F.; Horstman, D.H.

    1988-01-01

    Episodes occasionally occur when ambient ozone (O/sub 3/) levels remain at or near 0.12 ppm for more than 6 h. Small decrements in lung function have been reported following 2-h exposures to 0.12 ppm O/sub 3/. For short exposures to higher O/sub 3/ concentrations, lung function decrements are a function of exposure duration. Thus, we investigated the hypothesis that prolonged exposure to 0.12 ppm O/sub 3/ would result in progressively larger changes in respiratory function and symptoms over time. Ten nonsmoking males were exposed once to clean air and once to 0.12 ppm O/sub 3/ for 6.6 h. Exposures consisted of six 50-min exercise periods, each followed by 10-min rest and measurement; a 35-min lunch period followed by the third exercise period. Exercise ventilation averaged approximately 40 L/min. Forced expiratory and inspiratory spirometry and respiratory symptoms were measured prior to exposure and after each exercise. Airway reactivity to methacholine was determined after each exposure. After correcting for the air exposures, FEV 1.0 was found to decrease linearly during the O/sub 3/ exposure and was decreased by an average of 13.0 percent at the end of exposure. Decreases in FVC and FEF24-75% were also linear and averaged 8.3 and 17.4 percent, respectively, at the end of exposure. On forced inspiratory tests, the FIVC and FIV05 were decreased 12.6 and 20.7 percent, respectively. Increases in the symptom ratings of cough and pain on deep inspiration were observed with O/sub 3/ exposure but not with clean air. Airway reactivity to methacholine was approximately doubled following O/sub 3/ exposure.

  5. Pulmonary function and symptom responses after 6. 6-hour exposure to 0. 12-ppm ozone with moderate exercise (journal version)

    SciTech Connect (OSTI)

    Folinsbee, L.J.; Horstman, D.H.; McDonnell, W.F.

    1988-01-01

    Episodes occasionally occur when ambient ozone (O/sub 3/) levels remain at or near 0.12 ppm for more than 6 h. The hypothesis that prolonged exposure to 0.12 ppm O/sub 3/ would result in progressively larger changes in respiratory function and symptoms over time was tested. Ten nonsmoking males (18-35 yr) were exposed once to clear air (CA) and once to 0.12 pp, O/sub 3/ for 6.75 h. Exposures consisted of six 50-min exercise periods, each followed by 10-min rest and measurement; a 45-min lunch period followed the third exercise period. Exercise ventilation averaged approximately 40 1/min. Forced expiratory and inspiratory spirometry and respiratory symptoms were measured prior to exposure and after each exercise. Increases in the symptom ratings of cough and pain on deep inspiration were observed with O/sub 3/ exposure but not with CA. Airway reactivity to methacholine was approximately doubled following O/sub 3/ exposure. Spirometry results indicate that prolonged exposure to 0.12 ppm O/sub 3/ results in a marked increase in non-specific airway reactivity and progressive changes in respiratory function.

  6. Dark Matters

    ScienceCinema (OSTI)

    Joseph Silk

    2010-01-08

    One of the greatest mysteries in the cosmos is that it is mostly dark.  Astronomers and particle physicists today are seeking to unravel the nature of this mysterious, but pervasive dark matter which has profoundly influenced the formation of structure in the universe.  I will describe the complex interplay between galaxy formation and dark matter detectability and review recent attempts to measure particle dark matter by direct and indirect means.

  7. Matter in transition

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Anderson, Lara B.; Gray, James; Raghuram, Nikhil; Taylor, Washington

    2016-04-13

    In this study, we explore a novel type of transition in certain 6D and 4D quantum field theories, in which the matter content of the theory changes while the gauge group and other parts of the spectrum remain invariant. Such transitions can occur, for example, for SU(6) and SU(7) gauge groups, where matter fields in a three-index antisymmetric representation and the fundamental representation are exchanged in the transition for matter in the two-index antisymmetric representation. These matter transitions are realized by passing through superconformal theories at the transition point. We explore these transitions in dual F-theory and heterotic descriptions, wheremore » a number of novel features arise. For example, in the heterotic description the relevant 6D SU(7) theories are described by bundles on K3 surfaces where the geometry of the K3 is constrained in addition to the bundle structure. On the F-theory side, non-standard representations such as the three-index antisymmetric representation of SU(N) require Weierstrass models that cannot be realized from the standard SU(N) Tate form. We also briefly describe some other situations, with groups such as Sp(3), SO(12), and SU(3), where analogous matter transitions can occur between different representations. For SU(3), in particular, we find a matter transition between adjoint matter and matter in the symmetric representation, giving an explicit Weierstrass model for the F-theory description of the symmetric representation that complements another recent analogous construction.« less

  8. Dark Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Dark Matter Scientists are using the underground of the Waste Isolation Pilot Plant to try to solve the universe's major missing mass problem. He is enjoying his search They are searching for the presence of particles that may have mass but hardly interact with other matter. Based on observations of the relationships between mass and gravity and the speed of the stars and other cosmological systems, scientists believe that more than 90 percent of the universe's mass is "missing." A

  9. Dark Matter Theory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Dark Matter Theory Dark Matter Theory Understanding discoveries at the Energy, Intensity, and Cosmic Frontiers Get Expertise Rajan Gupta (505) 667-7664 Email Bruce Carlsten (505) ...

  10. Asymmetric dark matter

    SciTech Connect (OSTI)

    Kumar, Jason

    2014-06-24

    We review the theoretical framework underlying models of asymmetric dark matter, describe astrophysical constraints which arise from observations of neutron stars, and discuss the prospects for detecting asymmetric dark matter.

  11. Particulate Matter Aerosols

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    particulate matter aerosols Particulate Matter Aerosols The study of atmospheric aerosols is important because of its adverse effects on health, air quality, visibility, cultural heritage, and Earth's radiation balance. Techniques that can help better characterize particulate matter are required to better understand the constituents, causes and sources of particulate matter (PM) aerosols. Carbon is one of the main constituents of atmospheric aerosols. Radiocarbon (14C) measurement performed on

  12. Big Questions: Dark Matter

    ScienceCinema (OSTI)

    Lincoln, Don

    2014-08-07

    Carl Sagan's oft-quoted statement that there are "billions and billions" of stars in the cosmos gives an idea of just how much "stuff" is in the universe. However scientists now think that in addition to the type of matter with which we are familiar, there is another kind of matter out there. This new kind of matter is called "dark matter" and there seems to be five times as much as ordinary matter. Dark matter interacts only with gravity, thus light simply zips right by it. Scientists are searching through their data, trying to prove that the dark matter idea is real. Fermilab's Dr. Don Lincoln tells us why we think this seemingly-crazy idea might not be so crazy after all.

  13. Big Questions: Dark Matter

    SciTech Connect (OSTI)

    Lincoln, Don

    2013-12-05

    Carl Sagan's oft-quoted statement that there are "billions and billions" of stars in the cosmos gives an idea of just how much "stuff" is in the universe. However scientists now think that in addition to the type of matter with which we are familiar, there is another kind of matter out there. This new kind of matter is called "dark matter" and there seems to be five times as much as ordinary matter. Dark matter interacts only with gravity, thus light simply zips right by it. Scientists are searching through their data, trying to prove that the dark matter idea is real. Fermilab's Dr. Don Lincoln tells us why we think this seemingly-crazy idea might not be so crazy after all.

  14. Neutralino dark matter in BMSSM effective theory

    SciTech Connect (OSTI)

    Berg, Marcus; Edsj, Joakim; Lundstrm, Erik; Sjrs, Stefan; Gondolo, Paolo E-mail: edsjo@physto.se E-mail: erik@physto.se

    2009-08-01

    We study thermal neutralino dark matter in an effective field theory extension of the MSSM, called ''Beyond the MSSM'' (BMSSM) in Dine, Seiberg and Thomas (2007). In this class of effective field theories, the field content of the MSSM is unchanged, but the little hierarchy problem is alleviated by allowing small corrections to the Higgs/higgsino part of the Lagrangian. We perform parameter scans and compute the dark matter relic density. The light higgsino LSP scenario is modified the most; we find new regions of parameter space compared to the standard MSSM. This involves interesting interplay between the WMAP dark matter bounds and the LEP chargino bound. We also find some changes for gaugino LSPs, partly due to annihilation through a Higgs resonance, and partly due to coannihilation with light top squarks in models that are ruled in by the new effective terms.

  15. Ghost dark matter

    SciTech Connect (OSTI)

    Furukawa, Tomonori; Yokoyama, Shuichiro; Ichiki, Kiyotomo; Sugiyama, Naoshi; Mukohyama, Shinji E-mail: shu@a.phys.nagoya-u.ac.jp E-mail: naoshi@a.phys.nagoya-u.ac.jp

    2010-05-01

    We revisit ghost dark matter, the possibility that ghost condensation may serve as an alternative to dark matter. In particular, we investigate the Friedmann-Robertson-Walker (FRW) background evolution and the large-scale structure (LSS) in the ΛGDM universe, i.e. a late-time universe dominated by a cosmological constant and ghost dark matter. The FRW background of the ΛGDM universe is indistinguishable from that of the standard ΛCDM universe if M∼>1eV, where M is the scale of spontaneous Lorentz breaking. From the LSS we find a stronger bound: M∼>10eV. For smaller M, ghost dark matter would have non-negligible sound speed after the matter-radiation equality, and thus the matter power spectrum would significantly differ from observation. These bounds are compatible with the phenomenological upper bound M∼<100GeV known in the literature.

  16. Neutrinos and dark matter

    SciTech Connect (OSTI)

    Ibarra, Alejandro

    2015-07-15

    Neutrinos could be key particles to unravel the nature of the dark matter of the Universe. On the one hand, sterile neutrinos in minimal extensions of the Standard Model are excellent dark matter candidates, producing potentially observable signals in the form of a line in the X-ray sky. On the other hand, the annihilation or the decay of dark matter particles produces, in many plausible dark matter scenarios, a neutrino flux that could be detected at neutrino telescopes, thus providing non-gravitational evidence for dark matter. More conservatively, the non-observation of a significant excess in the neutrino fluxes with respect to the expected astrophysical backgrounds can be used to constrain dark matter properties, such as the self-annihilation cross section, the scattering cross section with nucleons and the lifetime.

  17. Part 1

    Office of Environmental Management (EM)

    1 Page 1-1 of 20 PART 1 - GENERAL PERMIT CONDITIONS 1.1. AUTHORITY This Permit is issued pursuant to the authority of the Secretary of the New Mexico Environment Department (Secretary) under the New Mexico Hazardous Waste Act (HWA), NMSA 1978, §§74- 4-1 through 74-4-14, in accordance with the New Mexico Hazardous Waste Management Regulations (HWMR), 20.4.1 NMAC. Pursuant to the Resource Conservation and Recovery Act (RCRA), 42 U.S.C. §§6901 to 6992k, and 40 CFR Part 271 and Part 272 Subpart

  18. Part 5

    Office of Environmental Management (EM)

    May 8, 2012 PERMIT PART 5 Page 5-1 of 11 PART 5 - GROUNDWATER DETECTION MONITORING 5.1. DETECTION MONITORING PROGRAM This Part specifies the requirements of the Detection Monitoring Program (DMP). The DMP shall establish background groundwater quality and monitor indicator parameters and waste constituents that provide a reliable indication of the presence of hazardous constituents in the groundwater, as required by 20.4.1.500 NMAC (incorporating 40 CFR §§264.97 and 264.98). The DMP consists

  19. Materials/Condensed Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Materials/Condensed Matter Materials/Condensed Matter Print Materials research provides the foundation on which the economic well being of our high-tech society rests. The impact of advanced materials ranges dramatically over every aspect of our modern world from the minutiae of daily life to the grand scale of our national economy. Invariably, however, breakthroughs to new technologies trace their origin both to fundamental research in the basic properties of condensed matter and to applied

  20. Dark Matter Theory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Dark Matter Theory Dark Matter Theory Understanding discoveries at the Energy, Intensity, and Cosmic Frontiers Get Expertise Rajan Gupta (505) 667-7664 Email Bruce Carlsten (505) 667-5657 Email Dark Matter Theory The existence of dark matter can be traced back to the pioneering discoveries of Fritz Zwicky and Jan Oort that the motion of galaxies in the Coma cluster, and of nearby stars in our own Galaxy, do not follow the expected motion based on Newton's law of gravity and the observed visible

  1. Cosmology with Mimetic Matter

    SciTech Connect (OSTI)

    Chamseddine, Ali H.; Mukhanov, Viatcheslav; Vikman, Alexander E-mail: viatcheslav.Mukhanov@lmu.de

    2014-06-01

    We consider minimal extensions of the recently proposed Mimetic Dark Matter and show that by introducing a potential for the mimetic non-dynamical scalar field we can mimic nearly any gravitational properties of the normal matter. In particular, the mimetic matter can provide us with inflaton, quintessence and even can lead to a bouncing nonsingular universe. We also investigate the behaviour of cosmological perturbations due to a mimetic matter. We demonstrate that simple mimetic inflation can produce red-tilted scalar perturbations which are largely enhanced over gravity waves.

  2. Science on Tap - Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Science on Tap - Matter Science on Tap - Matter WHEN: Feb 18, 2016 5:30 PM - 7:00 PM WHERE: UnQuarked Wine Room 145 Central Park Square, Los Alamos, New Mexico 87544 USA SPEAKER: Jack Shlachter CONTACT: Linda Anderman (505) 665-9196 CATEGORY: Bradbury INTERNAL: Calendar Login Event Description Mark your calendars for this event held every third Thursday from 5:30 to 7 p.m. A short presentation is followed by a lively discussion on a different subject each month. What's the Matter with Matter?

  3. Energy Matters Mailbag

    Broader source: Energy.gov [DOE]

    This edition of the mailbag tackles follow-up questions from our Energy Matters discussion on breaking our reliance on foreign oil.

  4. Magnetization of neutron matter

    SciTech Connect (OSTI)

    Bigdeli, M.

    2011-09-21

    In this paper, we compute magnetization of neutron matter at strong magnetic field using the lowest order constrained variational (LOCV) technique.

  5. Part 2

    Office of Environmental Management (EM)

    ... March 13, 2013 PERMIT PART 2 Page 2-6 of 21 2.3.3.6. PCB Waste Wastes with polychlorinated biphenyls (PCBs) not authorized under an EPA PCB waste disposal authorization are not ...

  6. PART I

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    B B-3 B.4 - ALLOWABILITY OF SUBCONTRACTOR FEE If the Contractor is part of a consortium, joint venture, andor other teaming arrangement, the team shall share in this Contract fee...

  7. Complex Dark Matter

    SciTech Connect (OSTI)

    Lincoln, Don

    2015-04-16

    After a century of study, scientists have come to the realization that the ordinary matter made of atoms is a minority in the universe. In order to explain observations, it appears that there exists a new and undiscovered kind of matter, called dark matter, that is five times more prevalent than ordinary matter. The evidence for this new matter’s existence is very strong, but scientists know only a little about its nature. In today’s video, Fermilab’s Dr. Don Lincoln talks about an exciting and unconventional idea, specifically that dark matter might have a very complex set of structures and interactions. While this idea is entirely speculative, it is an interesting hypothesis and one that scientists are investigating.

  8. PART I

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    C PART I SECTION C DESCRIPTION/SPECS./WORK STATEMENT TABLE OF CONTENTS PAGE NO. C.1 - INTRODUCTION C-1 C.2 - IMPLEMENTATION OF DOE'S MISSION FOR AMES C-2 C.3 - PERFORMANCE EXPECTATIONS, OBJECTIVES, AND MEASURES C-3 C.4 - STATEMENT OF WORK C-8 C.5 - PLANS AND REPORTS C-17 i Contract No. DE-AC02-07CH11358 Section C PART I SECTION C - DESCRIPTION/SPECS./WORK STATEMENT C.1 - INTRODUCTION This Performance-Based Management Contract (PBMC) is for the management and operation of the AMES Laboratory

  9. PART I

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    D PART I SECTION D PACKAGING AND MARKING TABLE OF CONTENTS PAGE NO. D.1 - PACKAGING D-1 D.2 - MARKING D-1 i Contract No. DE-AC02-07CH11358 Section D PART I SECTION D - PACKAGING AND MARKING D.1 - PACKAGING Preservation, packaging, and packing for shipment or mailing of all work delivered hereunder shall be in accordance with good commercial practice and adequate to ensure acceptance by common carrier and safe transportation at the most economical rates. D.2 - MARKING Each package, report or

  10. PART I

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    G Contract Modification No. 133 i PART I SECTION G CONTRACT ADMINISTRATION DATA TABLE OF CONTENTS PAGE NO. G.1- DOE CONTRACTING OFFICER G-1 G.2 - DOE CONTRACTING OFFICER'S REPRESENTATIVE (COR) G-1 G.3 - CONTRACT ADMINISTRATION G-1 G.4 - COST REPORTING PROCEDURES G-2 G.5 - INDIRECT CHARGES G-2 Contract No. DE-AC02-07CH11358 Section G Contract Modification No. 133 G-1 PART I SECTION G - CONTRACT ADMINISTRATION DATA G.1 - DOE CONTRACTING OFFICER For the definition of Contracting Officer see Federal

  11. PART I

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    B i PART I SECTION B SUPPLIES OR SERVICES AND PRICES/COSTS TABLE OF CONTENTS PAGE NO. B.1 - SERVICE BEING ACQUIRED B-1 B.2 - OBLIGATION OF FUNDS AND FINANCIAL LIMITATIONS B-1 B.3 - PERFORMANCE AND OTHER INCENTIVE FEES B-1 B.4 - ALLOWABILITY OF SUBCONTRACTOR FEE B-3 B.5 - PROVISIONAL PAYMENT OF PERFORMANCE FEE B-3 Contract No. DE-AC02-09CH11466 Section B B-1 PART I SECTION B - SUPPLIES OR SERVICES AND PRICES/COSTS B.1 - SERVICE BEING ACQUIRED The Contractor shall provide the personnel,

  12. PART I

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    DE-AC02-09CH11466 Section D i PART I SECTION D PACKAGING AND MARKING TABLE OF CONTENTS PAGE NO. D.1 - PACKAGING D-1 D.2 - MARKING D-1 Contract No. DE-AC02-09CH11466 Section D D-1...

  13. TSO-1004- In the Matter of Personnel Security Hearing

    Broader source: Energy.gov [DOE]

    The regulations governing the Individual’s eligibility are set forth at 10 C.F.R. Part 710, “Criteria and Procedures for Determining Eligibility for Access to Classified Matter or Special Nuclear...

  14. TBU-0110 - In the Matter of Greta Kathy Congable | Department...

    Energy Savers [EERE]

    As explained below, the Appeal should be granted in part and remanded for further processing. tbu0110.pdf (50.9 KB) More Documents & Publications TBH-0110 - In the Matter of Greta ...

  15. VWC-0001- In the Matter of Daniel L. Holsinger

    Broader source: Energy.gov [DOE]

    This case involves a complaint filed by Daniel Holsinger (Holsinger) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. The matter comes before me...

  16. VWC-0002- In the Matter of Daniel L. Holsinger

    Broader source: Energy.gov [DOE]

    This case involves a complaint filed by Daniel Holsinger (Holsinger) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. The matter comes before me...

  17. PART III

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Contract No. DE-AC02-09CH11466 Section J TOC i PART III List of Documents, Exhibits and Other Attachments Section J - List of Attachments Table of Contents Attachment No: Attachment: J.1 Appendix A - Advance Understandings on Human Resources J.2 Appendix B - Performance and Evaluation Measurement Plan J.3 Appendix C - Special Financial Institution Account Agreement J.4 Appendix D - Budget Program J.5 Appendix E - PPPL DOE (Lessee) Ingrants J.6 Appendix F - Contractor Resources, Commitments and

  18. Relativistic Laser-Matter Interactions

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Relativistic Laser-Matter Interactions Relativistic Laser-Matter Interactions Enabling the next generation of intense particle accelerators Contact Juan Fernandez (505) 667-6575 ...

  19. Materials/Condensed Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Materials/Condensed Matter Print Materials research provides the foundation on which the economic well being of our high-tech society rests. The impact of advanced materials ranges dramatically over every aspect of our modern world from the minutiae of daily life to the grand scale of our national economy. Invariably, however, breakthroughs to new technologies trace their origin both to fundamental research in the basic properties of condensed matter and to applied research aimed at manipulating

  20. Materials/Condensed Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Materials/Condensed Matter Print Materials research provides the foundation on which the economic well being of our high-tech society rests. The impact of advanced materials ranges dramatically over every aspect of our modern world from the minutiae of daily life to the grand scale of our national economy. Invariably, however, breakthroughs to new technologies trace their origin both to fundamental research in the basic properties of condensed matter and to applied research aimed at manipulating

  1. Part II

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    80 Thursday, No. 251 December 31, 2015 Part II Department of Defense General Services Administration National Aeronautics and Space Administration 48 CFR Chapter 1 Federal Acquisition Regulations; Final Rules VerDate Sep<11>2014 17:22 Dec 30, 2015 Jkt 238001 PO 00000 Frm 00001 Fmt 4717 Sfmt 4717 E:\FR\FM\31DER2.SGM 31DER2 tkelley on DSK3SPTVN1PROD with RULES2 81886 Federal Register / Vol. 80, No. 251 / Thursday, December 31, 2015 / Rules and Regulations DEPARTMENT OF DEFENSE GENERAL

  2. Cold fusion in condensed matter

    SciTech Connect (OSTI)

    Schommers, W.; Politis, C. )

    1989-01-01

    A model for cold fusion in condensed matter is proposed (cold fusion of deuterons in palladium). It is assumed that the palladium-deuterium system forms an alloy, i.e., it is assumed that Pd ions as well as d/sup +/ ions are embedded in an uniform background of negative charge (conduction electrons). The model is based on an interaction potential for deuterons in solid palladium which has been estimated by means of a theoretical picture well known in the physics of liquids. In particular, the following effects are possible: 1. Cold fusion in condensed matter can take place. 2. The observed energy should be larger than that given by the fusion reactions. 3. Hitherto unknown nuclear processes must not be postulated as reported by Fleischmann and Pons. 4. The deuterons are mobile. 5. The deuterons can form close-packed clusters, and in principle a fusion reaction can take place within such a cluster. 6. Not only /sup 3/He should be produced in Pd but possible /sup 4/He too. From their theoretical picture, it can be concluded that experimental results will be strongly dependent on the condition of the materials used in the experiments. This can possible explain that only a part of experiments could show up cold fusion. A well defined condition (lattice defects, different phases, impurities, etc.) of the materials is probably the most critical point in connection with the observation of cold fusion in condensed matter. The effect should also be influenced by lattice dilatations. Experiments with other materials instead of palladium (e.g. vanadium, titanium, lanthanide metals, and different alloys) should be probably more informative.

  3. Asymmetric twin Dark Matter

    SciTech Connect (OSTI)

    Farina, Marco

    2015-11-09

    We study a natural implementation of Asymmetric Dark Matter in Twin Higgs models. The mirroring of the Standard Model strong sector suggests that a twin baryon with mass around 5 GeV is a natural Dark Matter candidate once a twin baryon number asymmetry comparable to the SM asymmetry is generated. We explore twin baryon Dark Matter in two different scenarios, one with minimal content in the twin sector and one with a complete copy of the SM, including a light twin photon. The essential requirements for successful thermal history are presented, and in doing so we address some of the cosmological issues common to many Twin Higgs models. The required interactions we introduce predict signatures at direct detection experiments and at the LHC.

  4. Energy Matters - Fall 2002

    SciTech Connect (OSTI)

    2002-09-01

    Quarterly newsletter from DOE's Industrial Technologies Program to promote the use of energy-efficient industrial systems. This issue focus of this edition of the Energy Matters Newsletter is on energy and environmental issues. Read more about compressed air's role in productivity, making good motor decisions, and more.

  5. Energy Matters - Spring 2002

    SciTech Connect (OSTI)

    2002-03-01

    Quarterly newsletter from DOE's Industrial Technologies Program to promote the use of energy-efficient industrial systems. The focus of the Spring 2002 Issue of Energy Matters focuses on premium energy efficiency systems, with articles on new gas technologies, steam efficiency, the Augusta Newsprint Showcase, and more.

  6. Inflatable dark matter

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Davoudiasl, Hooman; Hooper, Dan; McDermott, Samuel

    2016-01-22

    Here, we describe a general scenario, dubbed “inflatable dark matter,” in which the density of dark matter particles can be reduced through a short period of late-time inflation in the early Universe. The overproduction of dark matter that is predicted within many, otherwise, well-motivated models of new physics can be elegantly remedied within this context. Thermal relics that would, otherwise, be disfavored can easily be accommodated within this class of scenarios, including dark matter candidates that are very heavy or very light. Furthermore, the nonthermal abundance of grand unified theory or Planck scale axions can be brought to acceptable levelsmore » without invoking anthropic tuning of initial conditions. A period of late-time inflation could have occurred over a wide range of scales from ~MeV to the weak scale or above, and could have been triggered by physics within a hidden sector, with small but not necessarily negligible couplings to the standard model.« less

  7. The Search for Dark Matter

    ScienceCinema (OSTI)

    Orrell, John

    2014-07-24

    More than 25 years ago, PNNL scientists began the first underground measurements searching for dark matter using specialized radiation detector technology. Dark matter is yet to be discovered says Physicist John L. Orrell.

  8. The Search for Dark Matter

    SciTech Connect (OSTI)

    Orrell, John

    2013-11-20

    More than 25 years ago, PNNL scientists began the first underground measurements searching for dark matter using specialized radiation detector technology. Dark matter is yet to be discovered says Physicist John L. Orrell.

  9. Part_3_Minority_Economic_Impact.pdf | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Part_3_Minority_Economic_Impact.pdf Part_3_Minority_Economic_Impact.pdf Part_3_Minority_Economic_Impact.pdf (437.63 KB) More Documents & Publications RFA-14-0002 - In the Matter of Highway Oil, Inc. Declaration Of Trust Founding Legislation - Office of Minority Economic Impact

  10. Direct search for dark matter

    SciTech Connect (OSTI)

    Yoo, Jonghee; /Fermilab

    2009-12-01

    Dark matter is hypothetical matter which does not interact with electromagnetic radiation. The existence of dark matter is only inferred from gravitational effects of astrophysical observations to explain the missing mass component of the Universe. Weakly Interacting Massive Particles are currently the most popular candidate to explain the missing mass component. I review the current status of experimental searches of dark matter through direct detection using terrestrial detectors.

  11. Rigid particulate matter sensor

    DOE Patents [OSTI]

    Hall, Matthew

    2011-02-22

    A sensor to detect particulate matter. The sensor includes a first rigid tube, a second rigid tube, a detection surface electrode, and a bias surface electrode. The second rigid tube is mounted substantially parallel to the first rigid tube. The detection surface electrode is disposed on an outer surface of the first rigid tube. The detection surface electrode is disposed to face the second rigid tube. The bias surface electrode is disposed on an outer surface of the second rigid tube. The bias surface electrode is disposed to face the detection surface electrode on the first rigid tube. An air gap exists between the detection surface electrode and the bias surface electrode to allow particulate matter within an exhaust stream to flow between the detection and bias surface electrodes.

  12. Inflatable Dark Matter

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Davoudiasl, Hooman; Hooper, Dan; McDermott, Samuel D.

    2016-01-22

    We describe a general scenario, dubbed “Inflatable Dark Matter”, in which the density of dark matter particles can be reduced through a short period of late-time inflation in the early universe. The overproduction of dark matter that is predicted within many otherwise well-motivated models of new physics can be elegantly remedied within this context, without the need to tune underlying parameters or to appeal to anthropic considerations. Thermal relics that would otherwise be disfavored can easily be accommodated within this class of scenarios, including dark matter candidates that are very heavy or very light. Furthermore, the non-thermal abundance of GUTmore » or Planck scale axions can be brought to acceptable levels, without invoking anthropic tuning of initial conditions. Additionally, a period of late-time inflation could have occurred over a wide range of scales from ~ MeV to the weak scale or above, and could have been triggered by physics within a hidden sector, with small but not necessarily negligible couplings to the Standard Model.« less

  13. Cosmology with matter diffusion

    SciTech Connect (OSTI)

    Calogero, Simone; Velten, Hermano E-mail: velten@cce.ufes.br

    2013-11-01

    We construct a viable cosmological model based on velocity diffusion of matter particles. In order to ensure the conservation of the total energy-momentum tensor in the presence of diffusion, we include a cosmological scalar field ? which we identify with the dark energy component of the universe. The model is characterized by only one new degree of freedom, the diffusion parameter ?. The standard ?CDM model can be recovered by setting ? = 0. If diffusion takes place (? > 0) the dynamics of the matter and of the dark energy fields are coupled. We argue that the existence of a diffusion mechanism in the universe may serve as a theoretical motivation for interacting models. We constrain the background dynamics of the diffusion model with Supernovae, H(z) and BAO data. We also perform a perturbative analysis of this model in order to understand structure formation in the universe. We calculate the impact of diffusion both on the CMB spectrum, with particular attention to the integrated Sachs-Wolfe signal, and on the matter power spectrum P(k). The latter analysis places strong constraints on the magnitude of the diffusion mechanism but does not rule out the model.

  14. Inflatable Dark Matter

    SciTech Connect (OSTI)

    Davoudiasl, Hooman; Hooper, Dan; McDermott, Samuel D.

    2015-07-30

    We describe a general scenario, dubbed “Inflatable Dark Matter”, in which the density of dark matter particles can be reduced through a short period of late-time inflation in the early universe. The overproduction of dark matter that is predicted within many otherwise well-motivated models of new physics can be elegantly remedied within this context, without the need to tune underlying parameters or to appeal to anthropic considerations. Thermal relics that would otherwise be disfavored can easily be accommodated within this class of scenarios, including dark matter candidates that are very heavy or very light. Furthermore, the non-thermal abundance of GUT or Planck scale axions can be brought to acceptable levels, without invoking anthropic tuning of initial conditions. Additionally, a period of late-time inflation could have occurred over a wide range of scales from ~ MeV to the weak scale or above, and could have been triggered by physics within a hidden sector, with small but not necessarily negligible couplings to the Standard Model.

  15. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Dispute Resolution ACREM Accountable Classified Removable Electronic Media AEA Atomic ... CLUP Comprehensive Land Use Plan CMPC Classified Matter Protection and Control CO ...

  16. _PART I - THE SCHEDULE

    National Nuclear Security Administration (NNSA)

    ... for all matters under the terms of the designation. ... or subcontractors to enter into or adhere to nor ... Participation in DOENNSA's Nuclear Emergency Search Team ...

  17. TBD-0075 -In the Matter of Jonathan Strausbaugh | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    5 -In the Matter of Jonathan Strausbaugh TBD-0075 -In the Matter of Jonathan Strausbaugh Pending before me is a consolidated Motion to Compel Discovery filed with the Office of Hearings and Appeals (OHA) on behalf of Jonathan K. Strausbaugh and Richard L. Rieckenberg (the complainants) by their attorney. This Motion relates to a hearing requested by the complainants under the Department of Energy's Contractor Employee Protection Program, 10 C.F.R. Part 708 (Part 708), in connection with the Part

  18. Discrete dark matter

    SciTech Connect (OSTI)

    Hirsch, M.; Morisi, S.; Peinado, E.; Valle, J. W. F. [AHEP Group, Institut de Fisica Corpuscular--C.S.I.C./Universitat de Valencia, Edificio Institutos de Paterna, Apartado 22085, E-46071 Valencia (Spain)

    2010-12-01

    We propose a new motivation for the stability of dark matter (DM). We suggest that the same non-Abelian discrete flavor symmetry which accounts for the observed pattern of neutrino oscillations, spontaneously breaks to a Z{sub 2} subgroup which renders DM stable. The simplest scheme leads to a scalar doublet DM potentially detectable in nuclear recoil experiments, inverse neutrino mass hierarchy, hence a neutrinoless double beta decay rate accessible to upcoming searches, while {theta}{sub 13}=0 gives no CP violation in neutrino oscillations.

  19. PPM Energy Inc | Open Energy Information

    Open Energy Info (EERE)

    Ownership W NERC Location WECC NERC WECC Yes Operates Generating Plant Yes Activity Wholesale Marketing Yes This article is a stub. You can help OpenEI by expanding it. Utility...

  20. Decoding dark matter in genes

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Decoding dark matter in genes Decoding dark matter in genes Possible future applications, for example, include making new cancer therapies based on how ribosomes differentiate in healthy versus cancerous tissue. February 19, 2016 Decoding dark matter in genes In 1994, researchers from Harvard and Stanford published a paper in which they described three mice: one was yellow and fat, one mottled and fat, and the last one was brown and lean. An ordinary image, except for one thing: despite being so

  1. Solving the Dark Matter Problem

    ScienceCinema (OSTI)

    Baltz, Ted

    2009-09-01

    Cosmological observations have firmly established that the majority of matter in the universe is of an unknown type, called 'dark matter'. A compelling hypothesis is that the dark matter consists of weakly interacting massive particles (WIMPs) in the mass range around 100 GeV. If the WIMP hypothesis is correct, such particles could be created and studied at accelerators. Furthermore they could be directly detected as the primary component of our galaxy. Solving the dark matter problem requires that the connection be made between the two. We describe some theoretical and experimental avenues that might lead to this connection.

  2. WBZ-14-0012 - In the Matter of UChicago Argonne LLC | Department of Energy

    Energy Savers [EERE]

    WBZ-14-0012 - In the Matter of UChicago Argonne LLC WBZ-14-0012 - In the Matter of UChicago Argonne LLC On July 21, 2015, an OHA Administrative Judge granted in part and denied in part a Motion for Summary Judgment filed by UChicago Argonne LLC (Argonne). In its Motion, Argonne sought dismissal of a Part 708 complaint filed by Jonathan McKay against the contractor on several grounds. After considering the parties' full briefing of this matter, the Administrative Judge determined that: (1)

  3. Organic Matter Management

    SciTech Connect (OSTI)

    Izaurralde, Roberto C.; Cerri, Carlos C.

    2002-01-01

    Soil organic matter (S)M) is an essential attribute of soil quality with a key role in soil conservation and sustainable agriculture. Many practices-some involving land use changes-have been shown to increase SOM and thus received considerable attention for their possible role in climate change mitigation. Carbon sequestration in managed soils occurs when there is a net removal of atmospheric CO2 because of the balance between carbon inputs (net primary productivity) and outputs (soil respiration, management-related C emissions). Soil C sequestration has the additional appeal that all its practices conform to principles of sustainable agriculture (e.g., reduced tillage, erosion control, diverse cropping systems, improved soil fertility). Long-term field experiments have been instrumental to increase our understanding of SOM dynamics. This chapter presents fundamental concepts to guide readers on the role of SOM in sustainable agriculture and climate change mitigation.

  4. TBU-0027 - In the Matter of Clint Olson | Department of Energy

    Office of Environmental Management (EM)

    27 - In the Matter of Clint Olson TBU-0027 - In the Matter of Clint Olson Clint Olson (the complainant or the employee), appeals the dismissal of his complaint of retaliation filed under 10 C.F.R. Part 708, the Department of Energy (DOE) Contractor Employee Protection Program. As explained below, the dismissal of the complaint should be reversed and the matter should be remanded for further processing to the Manager of the Employee Concerns Program (Manager) at the National Nuclear Security

  5. Constraints on particle dark matter from cosmic-ray antiprotons

    SciTech Connect (OSTI)

    Fornengo, N.; Vittino, A.; Maccione, L. E-mail: luca.maccione@lmu.de

    2014-04-01

    Cosmic-ray antiprotons represent an important channel for dark matter indirect-detection studies. Current measurements of the antiproton flux at the top of the atmosphere and theoretical determinations of the secondary antiproton production in the Galaxy are in good agreement, with no manifest deviation which could point to an exotic contribution in this channel. Therefore, antiprotons can be used as a powerful tool for constraining particle dark matter properties. By using the spectrum of PAMELA data from 50 MV to 180 GV in rigidity, we derive bounds on the dark matter annihilation cross section (or decay rate, for decaying dark matter) for the whole spectrum of dark matter annihilation (decay) channels and under different hypotheses of cosmic-rays transport in the Galaxy and in the heliosphere. For typical models of galactic propagation, the constraints are strong, setting a lower bound on the dark matter mass of a ''thermal'' relic at about 40–80 GeV for hadronic annihilation channels. These bounds are enhanced to about 150 GeV on the dark matter mass, when large cosmic-rays confinement volumes in the Galaxy are considered, and are reduced to 3–4 GeV for annihilation to light quarks (no bound for heavy-quark production) when the confinement volume is small. Bounds for dark matter lighter than few tens of GeV are due to the low energy part of the PAMELA spectrum, an energy region where solar modulation is relevant: to this aim, we have implemented a detailed solution of the transport equation in the heliosphere, which allowed us not only to extend bounds to light dark matter, but also to determine the uncertainty on the constraints arising from solar modulation modelling. Finally, we estimate the impact of soon-to-come AMS-02 data on the antiproton constraints.

  6. Nuclear-matter--quark-matter phase diagram with strangeness

    SciTech Connect (OSTI)

    Barz, H. W.; Friman, B. L.; Knoll, J.; Schulz, H.

    1989-07-01

    A phenomenological equation of state of strongly interacting matter, including strange degrees of freedom, is presented. It is shown that the hyperon and kaon interactions must be included, in order to obtain a reasonable description of the deconfinement transition at high baryon densities. The consequences of kaon condensation on the nuclear-matter--quark-matter phase diagram are explored. The relative particle abundances obtained in an isentropic expansion of a blob of quark-gluon plasma are presented for different initial conditions. Implications for ultrarelativistic heavy-ion collisions are briefly discussed.

  7. Probing gravitational dark matter

    SciTech Connect (OSTI)

    Ren, Jing; He, Hong-Jian

    2015-03-27

    So far all evidences of dark matter (DM) come from astrophysical and cosmological observations, due to the gravitational interactions of DM. It is possible that the true DM particle in the universe joins gravitational interactions only, but nothing else. Such a Gravitational DM (GDM) may act as a weakly interacting massive particle (WIMP), which is conceptually simple and attractive. In this work, we explore this direction by constructing the simplest scalar GDM particle χ{sub s}. It is a ℤ{sub 2} odd singlet under the standard model (SM) gauge group, and naturally joins the unique dimension-4 interaction with Ricci curvature, ξ{sub s}χ{sub s}{sup 2}R, where ξ{sub s} is the dimensionless nonminimal coupling. We demonstrate that this gravitational interaction ξ{sub s}χ{sub s}{sup 2}R, together with Higgs-curvature nonminimal coupling term ξ{sub h}H{sup †}HR, induces effective couplings between χ{sub s}{sup 2} and SM fields, and can account for the observed DM thermal relic abundance. We analyze the annihilation cross sections of GDM particles and derive the viable parameter space for realizing the DM thermal relic density. We further study the direct/indirect detections and the collider signatures of such a scalar GDM. These turn out to be highly predictive and testable.

  8. WBU-15-0007 - In the Matter of Stacey Kittner | Department of Energy

    Energy Savers [EERE]

    7 - In the Matter of Stacey Kittner WBU-15-0007 - In the Matter of Stacey Kittner On July 7, 2015, the OHA issued a decision granting in part a jurisdictional appeal filed by Ms. Stacey Kittner, a former senior member of the technical staff of Sandia National Laboratory (Sandia). Ms. Kittner appealed the National Nuclear Security Administration's (NNSA) June 4, 2015, dismissal of a whistleblower complaint that she filed under 10 CFR Part 708, the DOE Contractor Employee Protection Program. OHA

  9. TBD-0073 - In the Matter of Richard L. Rieckenberg | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    3 - In the Matter of Richard L. Rieckenberg TBD-0073 - In the Matter of Richard L. Rieckenberg Pending before me is a consolidated Motion to Compel Discovery filed with the Office of Hearings and Appeals (OHA) on behalf of Jonathan K. Strausbaugh and Richard L. Rieckenberg (the complainants) by their attorney. This Motion relates to a hearing requested by the complainants under the Department of Energy's Contractor Employee Protection Program, 10 C.F.R. Part 708 (Part 708), in connection with

  10. PSH-14-0056 - In the Matter of Personnel Security | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    56 - In the Matter of Personnel Security PSH-14-0056 - In the Matter of Personnel Security On September 11, 2014, an OHA Administrative Judge (AJ) issued a Decision in which she concluded that the DOE should not restore an individual's suspended DOE access authorization. A DOE Operations Office referred the individual to administrative review under 10 C.F.R. Part 710, citing as security concerns under 10 C.F.R. Part 710 information pertaining to the Individual's mental condition, specifically

  11. PSH-14-0090 - In the Matter of Personnel Security | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    0 - In the Matter of Personnel Security PSH-14-0090 - In the Matter of Personnel Security On December 23 2014, an OHA Administrative Judge (AJ) issued a Decision in which she concluded that the DOE should not restore an individual's access authorization. A DOE Operations Office referred the individual to administrative review under 10 C.F.R. Part 710, citing as security concerns under 10 C.F.R. Part 710 the individual's falsifications, omissions, or misrepresentations on a security

  12. MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; SOLID STATE...

    Office of Scientific and Technical Information (OSTI)

    Open problems in condensed matter physics, 1987 Falicov, L.M. 75 CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; SOLID STATE PHYSICS; RESEARCH PROGRAMS;...

  13. Energy Matters LLC | Open Energy Information

    Open Energy Info (EERE)

    Name: Energy Matters LLC Place: Santa Rosa, California Zip: 95402 Sector: Renewable Energy Product: Energy Matters specialises in software tools for the renewable energy...

  14. Physical Protection of Classified Matter

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    1988-02-03

    The order establishes policy and objectives for physical protection of classified matter. This directive does not cancel another directive. Chg 1, 7-30-93. Canceled by 5632.1C.

  15. Energy Matters: Our Energy Independence

    Broader source: Energy.gov [DOE]

    In this installment of the livechat series "Energy Matters," Dr. Arun Majumdar takes questions from the public about the investments we're making today that will move us off of foreign oil and...

  16. Integrated coherent matter wave circuits

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Ryu, C.; Boshier, M. G.

    2015-09-21

    An integrated coherent matter wave circuit is a single device, analogous to an integrated optical circuit, in which coherent de Broglie waves are created and then launched into waveguides where they can be switched, divided, recombined, and detected as they propagate. Applications of such circuits include guided atom interferometers, atomtronic circuits, and precisely controlled delivery of atoms. We report experiments demonstrating integrated circuits for guided coherent matter waves. The circuit elements are created with the painted potential technique, a form of time-averaged optical dipole potential in which a rapidly moving, tightly focused laser beam exerts forces on atoms through theirmoreelectric polarizability. Moreover, the source of coherent matter waves is a BoseEinstein condensate (BEC). Finally, we launch BECs into painted waveguides that guide them around bends and form switches, phase coherent beamsplitters, and closed circuits. These are the basic elements that are needed to engineer arbitrarily complex matter wave circuitry.less

  17. Relativistic Laser-Matter Interactions

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Relativistic Laser-Matter Interactions Relativistic Laser-Matter Interactions Enabling the next generation of intense particle accelerators Contact Juan Fernandez (505) 667-6575 Email Short-pulse ion acceleration The Trident facility is a world-class performer in the area of ion acceleration from laser-solid target interactions. Trident has demonstrated over 100 MeV protons at intensities of 8x1020 W/cm2 with efficiencies approaching 5%. These intense relativistic interactions can be diagnosed

  18. Energy Matters | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Matters Energy Matters July 25, 2011 - 1:04pm Addthis On Wednesday, January 26th, Secretary Chu held an online town hall to discuss President Obama's clean energy and innovation agenda. Read a recap and watch video from the full event here. Addthis Related Articles WEDNESDAY: Secretary Chu to Host Live Chat on Clean Energy and Innovation Vice President Biden Kicks Off Five Days of Earth Day Activities with Announcement of Major New Energy Efficiency Effort Energy Secretary Steven Chu to Travel

  19. Condensed Matter and Magnet Science

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    CMMS Condensed Matter and Magnet Science The group has a distinguished history of applying cutting-edge condensed matter physics research and high magnetic field science to mission-relevant materials challenges as well as fundamental investigations of emergent physical phenomena. Contact Us Group Leader Michael Hundley Email Deputy Group Leader Chuck Mielke Email NHMFL-PFF Director Chuck Mielke Email Deputy NHMFL-PFF Director Ross McDonald Email Group Office (505) 667-4838 NHMFL Office (505)

  20. Strongly interacting parton matter equilibration

    SciTech Connect (OSTI)

    Ozvenchuk, V.; Linnyk, O.; Bratkovskaya, E.; Gorenstein, M.; Cassing, W.

    2012-07-15

    We study the kinetic and chemical equilibration in 'infinite' parton matter within the Parton-Hadron-String Dynamics transport approach. The 'infinite' matter is simulated within a cubic box with periodic boundary conditions initialized at different energy densities. Particle abundances, kinetic energy distributions, and the detailed balance of the off-shell quarks and gluons in the strongly-interacting quarkgluon plasma are addressed and discussed.

  1. Dark matter beams at LBNF

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Coloma, Pilar; Dobrescu, Bogdan A.; Frugiuele, Claudia; Harnik, Roni

    2016-04-08

    High-intensity neutrino beam facilities may produce a beam of light dark matter when protons strike the target. Searches for such a dark matter beam using its scattering in a nearby detector must overcome the large neutrino background. We characterize the spatial and energy distributions of the dark matter and neutrino beams, focusing on their differences to enhance the sensitivity to dark matter. We find that a dark matter beam produced by a Zmore » $$^{'}$$ boson in the GeV mass range is both broader and more energetic than the neutrino beam. The reach for dark matter is maximized for a detector sensitive to hard neutral-current scatterings, placed at a sizable angle off the neutrino beam axis. In the case of the Long-Baseline Neutrino Facility (LBNF), a detector placed at roughly 6 degrees off axis and at a distance of about 200 m from the target would be sensitive to Z$$^{'}$$ couplings as low as 0.05. This search can proceed symbiotically with neutrino measurements. We also show that the MiniBooNE and MicroBooNE detectors, which are on Fermilab’s Booster beamline, happen to be at an optimal angle from the NuMI beam and could perform searches with existing data. As a result, this illustrates potential synergies between LBNF and the short-baseline neutrino program if the detectors are positioned appropriately.« less

  2. WIMP Dark Matter Limit-Direct Detection Data and Sensitivity Plots from the Cryogenic Dark Matter Search II and the University of California at Santa Barbara

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Expectations for non-baryonic dark matter are founded principally in Big Bang nucleosynthesis calculations, which indicate that the missing mass of the universe is not likely to be baryonic. The supersymmetric standard model (SUSY) offers a promising framework for expectations of particle species which could satisfy the observed properties of dark matter. WIMPs are the most likely SUSY candidate for a dark matter particle. The High Energy Physics Group at University of California, Santa Barbara, is part of the CDMSII Collaboration and have provided the Interactive Plotter for WIMP Dark Matter Limit-Direct Detection Data on their website. They invite other collaborations working on dark matter research to submit datasets and, as a result, have more than 150 data sets now available for use with the plotting tool. The published source of the data is provided with each data set.

  3. Distinct optical properties of relativistically degenerate matter

    SciTech Connect (OSTI)

    Akbari-Moghanjoughi, M.

    2014-06-15

    In this paper, we use the collisional quantum magnetohydrodynamic (CQMHD) model to derive the transverse dielectric function of a relativistically degenerate electron fluid and investigate various optical parameters, such as the complex refractive index, the reflection and absorption coefficients, the skin-depth and optical conductivity. In this model we take into accounts effects of many parameters such as the atomic-number of the constituent ions, the electron exchange, electron diffraction effect and the electron-ion collisions. Study of the optical parameters in the solid-density, the warm-dense-matter, the big-planetary core, and the compact star number-density regimes reveals that there are distinct differences between optical characteristics of the latter and the former cases due to the fundamental effects of the relativistic degeneracy and other quantum mechanisms. It is found that in the relativistic degeneracy plasma regime, such as found in white-dwarfs and neutron star crusts, matter possess a much sharper and well-defined step-like reflection edge beyond the x-ray electromagnetic spectrum, including some part of gamma-ray frequencies. It is also remarked that the magnetic field intensity only significantly affects the plasma reflectivity in the lower number-density regime, rather than the high density limit. Current investigation confirms the profound effect of relativistic degeneracy on optical characteristics of matter and can provide an important plasma diagnostic tool for studying the physical processes within the wide scope of quantum plasma regimes be it the solid-density, inertial-confined, or astrophysical compact stars.

  4. Stocks of Distillate Fuel Oil Greater Than 15 ppm to 500 ppm Sulfur

    Gasoline and Diesel Fuel Update (EIA)

    8,090 9,314 9,448 9,647 9,783 9,706 1993-2016 PADD 1 5,171 6,277 6,929 6,828 7,018 6,801 1993-2016 New England 2,996 3,690 4,059 3,917 3,986 4,042 1993-2016 Central Atlantic 1,863 2,272 2,447 2,491 2,627 2,435 1993-2016 Lower Atlantic 313 315 423 420 405 323 1993-2016 PADD 2 351 427 439 408 410 427 1993-2016 PADD 3 2,093 2,128 1,579 1,929 1,813 1,925 1993-2016 PADD 4 130 133 136 127 137 143 1993-2016 PADD 5 345 349 366 355 405 409

  5. Beryllium Related Matter

    SciTech Connect (OSTI)

    Gaylord, R F

    2008-12-23

    In recent months, LLNL has identified, commenced, and implemented a series of interim controls, compensatory measures, and initiatives to ensure worker safety, and improve safety processes with regards to potential worker exposure to beryllium. Many of these actions have been undertaken in response to the NNSA Independent Review (COR-TS-5/15/2008-8550) received by LLNL in November of 2008. Others are the result of recent discoveries, events or incidents, and lessons learned, or were scheduled corrective actions from earlier commitments. Many of these actions are very recent in nature, or are still in progress, and vary in the formality of implementation. Actions are being reviewed for effectiveness as they progress. The documentation of implementation, and review of effectiveness, when appropriate, of these actions will be addressed as part of the formal Corrective Action Plan addressing the Independent Review. The mitigating actions taken fall into the following categories: (1) Responses to specific events/concerns; (2) Development of interim controls; (3) Review of ongoing activities; and (4) Performance improvement measures.

  6. Dark Matter Constraints from a Cosmic Index of Refraction

    SciTech Connect (OSTI)

    Gardner, Susan; Latimer, David C.

    2009-04-01

    The dark-matter candidates of particle physics invariably possess electromagnetic interactions, if only via quantum fluctuations. Taken en masse, dark matter can thus engender an index of refraction which deviates from its vacuum value. Its presence is signaled through frequency-dependent effects: the real part yields dispersive effects in propagation, and the imaginary part yields such in attenuation. We discuss theoretical constraints on the expansion of the index of refraction with frequency, the physical interpretation of the terms, and the particular observations needed to isolate its coefficients. This, with the advent of new opportunities to view gamma-ray bursts at cosmological distance scales, gives us a new probe of dark matter. As a first application we use the time delay determined from radio afterglow observations of gamma-ray bursts to limit the charge-to-mass ratio of dark matter to |{var_epsilon}|/M < 1.8 x 10{sup -5} eV{sup -1} at 95% CL.

  7. Dark matter in 3D

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Alves, Daniele S. M.; El Hedri, Sonia; Wacker, Jay G.

    2016-03-21

    We discuss the relevance of directional detection experiments in the post-discovery era and propose a method to extract the local dark matter phase space distribution from directional data. The first feature of this method is a parameterization of the dark matter distribution function in terms of integrals of motion, which can be analytically extended to infer properties of the global distribution if certain equilibrium conditions hold. The second feature of our method is a decomposition of the distribution function in moments of a model independent basis, with minimal reliance on the ansatz for its functional form. We illustrate our methodmore » using the Via Lactea II N-body simulation as well as an analytical model for the dark matter halo. Furthermore, we conclude that O(1000) events are necessary to measure deviations from the Standard Halo Model and constrain or measure the presence of anisotropies.« less

  8. Dark matter and gauged flavor symmetries

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Bishara, Fady; Greljo, Admir; Kamenik, Jernej F.; Stamou, Emmanuel; Zupan, Jure

    2015-12-21

    We investigate the phenomenology of flavored dark matter (DM). DM stability is guaranteed by an accidental Z3 symmetry, a subgroup of the standard model (SM) flavor group that is not broken by the SM Yukawa interactions. We consider an explicit realization where the quark part of the SM flavor group is fully gauged. If the dominant interactions between DM and visible sector are through flavor gauge bosons, as we show for Dirac fermion flavored DM, then the DM mass is bounded between roughly 0.5 TeV and 5 TeV if the DM multiplet mass is split only radiatively. In general, however,more » no such relation exists. We demonstrate this using scalar flavored DM where the main interaction with the SM is through the Higgs portal. For both cases we derive constraints from flavor, cosmology, direct and indirect DM detection, and collider searches.« less

  9. Dark matter and gauged flavor symmetries

    SciTech Connect (OSTI)

    Bishara, Fady; Greljo, Admir; Kamenik, Jernej F.; Stamou, Emmanuel; Zupan, Jure

    2015-12-21

    We investigate the phenomenology of flavored dark matter (DM). DM stability is guaranteed by an accidental Z3 symmetry, a subgroup of the standard model (SM) flavor group that is not broken by the SM Yukawa interactions. We consider an explicit realization where the quark part of the SM flavor group is fully gauged. If the dominant interactions between DM and visible sector are through flavor gauge bosons, as we show for Dirac fermion flavored DM, then the DM mass is bounded between roughly 0.5 TeV and 5 TeV if the DM multiplet mass is split only radiatively. In general, however, no such relation exists. We demonstrate this using scalar flavored DM where the main interaction with the SM is through the Higgs portal. For both cases we derive constraints from flavor, cosmology, direct and indirect DM detection, and collider searches.

  10. EVM Subject Matter Experts | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Management » EVM Subject Matter Experts EVM Subject Matter Experts Name Title Office * Phone Email Melvin Frank Chief, Project Management Policy and Systems PM-30 202-586-5519 Send Email David Kester EVMS Subject Matter Expert PM-30 202-586-4342 Send Email Robert Loop EVMS Subject Matter Expert PM-30 202-287-1324 Send Email Karen Urschel (CONTR) EVMS Subject Matter Expert PM-30 260-417-2184 Send Email Buck Wilkerson (CONTR) Planning and Scheduling Subject Matter Expert PM-30 678-360-3161 Send

  11. Apparatus for particulate matter analysis

    DOE Patents [OSTI]

    Gundel, Lara A.; Apte, Michael G.; Hansen, Anthony D.; Black, Douglas R.

    2007-01-30

    The apparatus described herein is a miniaturized system for particle exposure assessment (MSPEA) for the quantitative measurement and qualitative identification of particulate content in gases. The present invention utilizes a quartz crystal microbalance (QCM) or other mass-sensitive temperature compensated acoustic wave resonator for mass measurement. Detectors and probes and light sources are used in combination for the qualitative determination of particulate matter.

  12. Z-portal dark matter

    SciTech Connect (OSTI)

    Arcadi, Giorgio; Mambrini, Yann; Richard, Francois

    2015-03-11

    We propose to generalize the extensions of the Standard Model where the Z boson serves as a mediator between the Standard Model sector and the dark sector χ. We show that, like in the Higgs portal case, the combined constraints from the recent direct searches restrict severely the nature of the coupling of the dark matter to the Z boson and set a limit m{sub χ}≳200 GeV (except in a very narrow region around the Z-pole region). Using complementarity between spin dependent, spin independent and FERMI limits, we predict the nature of this coupling, more specifically the axial/vectorial ratio that respects a thermal dark matter coupled through a Z-portal while not being excluded by the current observations. We also show that the next generation of experiments of the type LZ or XENON1T will test Z-portal scenario for dark matter mass up to 2 TeV. The condition of a thermal dark matter naturally predicts the spin-dependent scattering cross section on the neutron to be σ{sub χn}{sup SD}≃10{sup −40} cm{sup 2}, which then becomes a clear prediction of the model and a signature testable in the near future experiments.

  13. Wino dark matter under siege

    SciTech Connect (OSTI)

    Cohen, Timothy; Lisanti, Mariangela; Pierce, Aaron; Slatyer, Tracy R. E-mail: mlisanti@princeton.edu E-mail: tslatyer@mit.edu

    2013-10-01

    A fermion triplet of SU(2){sub L} a wino is a well-motivated dark matter candidate. This work shows that present-day wino annihilations are constrained by indirect detection experiments, with the strongest limits coming from H.E.S.S. and Fermi. The bounds on wino dark matter are presented as a function of mass for two scenarios: thermal (winos constitute a subdominant component of the dark matter for masses less than 3.1 TeV) and non-thermal (winos comprise all the dark matter). Assuming the NFW halo model, the H.E.S.S. search for gamma-ray lines excludes the 3.1 TeV thermal wino; the combined H.E.S.S. and Fermi results completely exclude the non-thermal scenario. Uncertainties in the exclusions are explored. Indirect detection may provide the only probe for models of anomaly plus gravity mediation where the wino is the lightest superpartner and scalars reside at the 100 TeV scale.

  14. Dark matter as a ghost free conformal extension of Einstein theory

    SciTech Connect (OSTI)

    Barvinsky, A.O.

    2014-01-01

    We discuss ghost free models of the recently suggested mimetic dark matter theory. This theory is shown to be a conformal extension of Einstein general relativity. Dark matter originates from gauging out its local Weyl invariance as an extra degree of freedom which describes a potential flow of the pressureless perfect fluid. For a positive energy density of this fluid the theory is free of ghost instabilities, which gives strong preference to stable configurations with a positive scalar curvature and trace of the matter stress tensor. Instabilities caused by caustics of the geodesic flow, inherent in this model, serve as a motivation for an alternative conformal extension of Einstein theory, based on the generalized Proca vector field. A potential part of this field modifies the inflationary stage in cosmology, whereas its rotational part at the post inflationary epoch might simulate rotating flows of dark matter.

  15. Do New Technologies Matter? | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Do New Technologies Matter? Do New Technologies Matter? February 12, 2015 - 2:07pm Addthis Pat Adams Pat Adams Digital Content Specialist, Office of Public Affairs Learn More Learn ...

  16. Cold quark matter in compact stars

    SciTech Connect (OSTI)

    Franzon, B.; Fogaca, D. A.; Navarra, F. S.; Horvath, J. E.

    2013-03-25

    We used an equation of state for the cold quark matter to the study of properties of quark stars. We also discuss the absolute stability of quark matter and compute the mass-radius relation for self-bound stars.

  17. Policy Matters Ohio | Open Energy Information

    Open Energy Info (EERE)

    Matters Ohio Jump to: navigation, search Name: Policy Matters Ohio Address: 3631 Perkins Avenue - Suite 4C-East Place: Cleveland, Ohio Zip: 44114 Website: www.policymattersohio.org...

  18. Science On Tap - Matter over. Antimatter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Science On Tap - Matter over Antimatter Science On Tap - Matter over. Antimatter WHEN: Aug 20, 2015 5:30 PM - 7:00 PM WHERE: UnQuarked Wine Room 145 Central Park Square, Los...

  19. Mentoring Matters: Engaging Students through Science and Arts...

    Office of Environmental Management (EM)

    Mentoring Matters: Engaging Students through Science and Arts Mentoring Matters: Engaging Students through Science and Arts April 22, 2016 - 11:48am Addthis Mentoring Matters: ...

  20. MPA Materials Matter December 2015 (Technical Report) | SciTech...

    Office of Scientific and Technical Information (OSTI)

    MPA Materials Matter December 2015 Citation Details In-Document Search Title: MPA Materials Matter December 2015 This is the December 2015 issue of the MPA Materials Matter ...

  1. Dark matter in a bouncing universe

    SciTech Connect (OSTI)

    Cheung, Yeuk-Kwan E.; Kang, Jin U; Li, Changhong E-mail: jin.u.kang2@gmail.com

    2014-11-01

    We investigate a new scenario of dark matter production in a bouncing universe, in which dark matter was produced completely out of equilibrium in the contracting as well as expanding phase. We explore possibilities of using dark matter as a probe of the bouncing universe, focusing on the relationship between a critical temperature of the bouncing universe and the present relic abundance of dark matter.

  2. The equation of state of nuclear matter

    SciTech Connect (OSTI)

    Gandolfi, Stefano; Carlson, Joseph Allen

    2015-06-30

    A brief status report of research on equation of state (EOS) of nuclear matter is provided, along with two graphs.

  3. Dark Matter Annihilation at the Galactic Center

    SciTech Connect (OSTI)

    Linden, Timothy Ryan

    2013-06-01

    Observations by the WMAP and PLANCK satellites have provided extraordinarily accurate observations on the densities of baryonic matter, dark matter, and dark energy in the universe. These observations indicate that our universe is composed of approximately ve times as much dark matter as baryonic matter. However, e orts to detect a particle responsible for the energy density of dark matter have been unsuccessful. Theoretical models have indicated that a leading candidate for the dark matter is the lightest supersymmetric particle, which may be stable due to a conserved R-parity. This dark matter particle would still be capable of interacting with baryons via weak-force interactions in the early universe, a process which was found to naturally explain the observed relic abundance of dark matter today. These residual annihilations can persist, albeit at a much lower rate, in the present universe, providing a detectable signal from dark matter annihilation events which occur throughout the universe. Simulations calculating the distribution of dark matter in our galaxy almost universally predict the galactic center of the Milky Way Galaxy (GC) to provide the brightest signal from dark matter annihilation due to its relative proximity and large simulated dark matter density. Recent advances in telescope technology have allowed for the rst multiwavelength analysis of the GC, with suitable e ective exposure, angular resolution, and energy resolution in order to detect dark matter particles with properties similar to those predicted by the WIMP miracle. In this work, I describe ongoing e orts which have successfully detected an excess in -ray emission from the region immediately surrounding the GC, which is di cult to describe in terms of standard di use emission predicted in the GC region. While the jury is still out on any dark matter interpretation of this excess, I describe several related observations which may indicate a dark matter origin. Finally, I discuss the

  4. Operations & Maintenance Best Practices Guide: Front Matter

    Broader source: Energy.gov [DOE]

    Guide describes the front matter of the Operations and Maintenance Best Practices: a Guide to Achieving Operational Efficiency.

  5. VBH-0062 - In the Matter of Sue Rice Gossett | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    VBH-0062 - In the Matter of Sue Rice Gossett VBH-0062 - In the Matter of Sue Rice Gossett This Initial Agency Decision concerns a whistleblower complaint filed by Sue Rice Gossett (Gossett) against her former employer, the Safety and Ecology Corporation (SEC), under the Department of Energy's (DOE) Contractor Employee Protection Program, which is codified at 10 C.F.R. Part 708. SEC is a sub-contractor of Bechtel Jacobs Corporation (BJC), the DOE's Managing Contractor at the Portsmouth Site in

  6. VBZ-0062 - In the Matter of Sue Rice Gossett | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    VBZ-0062 - In the Matter of Sue Rice Gossett VBZ-0062 - In the Matter of Sue Rice Gossett This Initial Agency Decision concerns a whistleblower complaint filed by Sue Rice Gossett (Gossett) against her former employer, the Safety and Ecology Corporation (SEC), under the Department of Energy's (DOE) Contractor Employee Protection Program, which is codified at 10 C.F.R. Part 708. SEC is a sub-contractor of Bechtel Jacobs Corporation (BJC), the DOE's Managing Contractor at the Portsmouth Site in

  7. VEE-0054 - In the Matter of Amana Appliances | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    54 - In the Matter of Amana Appliances VEE-0054 - In the Matter of Amana Appliances This Decision and Order considers an Application for Exception filed by Amana Appliances (Amana), seeking exception relief from the provisions of 10 C.F.R. Part 430, Energy Conservation Program for Consumer Products: Energy Conservation Standards for Refrigerators, Refrigerator-Freezers and Freezers (Refrigerator Efficiency Standards). In its exception request, Amana asserts that the firm would suffer a

  8. VEE-0075 - In the Matter of Viking Range Corporation | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    5 - In the Matter of Viking Range Corporation VEE-0075 - In the Matter of Viking Range Corporation This Decision and Order considers an Application for Exception filed by Viking Range Corporation (Viking) seeking exception relief from the provisions of 10 C.F.R. Part 430, Energy Conservation Program for Consumer Products: Energy Conservation Standards for Refrigerators, Refrigerator-Freezers and Freezers (Refrigerator Efficiency Standards). In its exception request, Viking asserts that the firm

  9. EXC-11-0001 - In the Matter of BSH Home Appliances Corporation | Department

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    of Energy 1-0001 - In the Matter of BSH Home Appliances Corporation EXC-11-0001 - In the Matter of BSH Home Appliances Corporation On January 4, 2012, OHA issued a decision granting an Application for Exception filed by BSH Home Appliances Corporation (BSH). In its Application, the BSH sought relief from the provisions of 10 C.F.R. Part 430, Energy Conservation Program for Consumer Products: Energy Conservation Standards for Refrigerators, Refrigerator-Freezers and Freezers (Refrigerator

  10. EXC-15-0001 - In the Matter of Reuland Electric Co. | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    5-0001 - In the Matter of Reuland Electric Co. EXC-15-0001 - In the Matter of Reuland Electric Co. On March 25, 2016, OHA issued a decision denying an Application for Exception filed by Reuland Electric Co. (Reuland). In its Application, Reuland sought exception relief from the provisions of 10 CFR Part 431, Energy Conservation Program: Energy Conservation Standards for Commercial and Industrial Electric Blowers, 79 Fed. Reg. 30934 (2014) (Electric Motor Efficiency Standards), effective July 28,

  11. EXC-16-0010 - In the Matter of Visual Sound LLC dba Truetone | Department

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    of Energy 10 - In the Matter of Visual Sound LLC dba Truetone EXC-16-0010 - In the Matter of Visual Sound LLC dba Truetone On July 5, 2016, OHA granted an Application for Exception filed by Visual Sound LLC dba Truetone (Truetone). Truetone, a manufacturer of specialized noise free external power supplies (EPSs) for musical equipment, requested exception relief from the applicable provisions of 10 CFR Part 430, Energy Conservation Program: Energy Conservation Standards for External Power

  12. TEE-0074 - In the Matter of GE Appliances & Lighting | Department of Energy

    Energy Savers [EERE]

    4 - In the Matter of GE Appliances & Lighting TEE-0074 - In the Matter of GE Appliances & Lighting This Decision and Order considers an Application for Exception filed by GE Appliances & Lighting (GE) seeking exception relief from the provision of 10 C.F.R. Part 430, Energy Conservation Program for Consumer Products: Energy Conservation Standards for Refrigerators, Refrigerator-Freezers and Freezers (Refrigerator Efficiency Standards). In its exception request, GE asserts that the

  13. WBA-14-0006 - In the Matter of Anthony T. Rivera | Department of Energy

    Energy Savers [EERE]

    6 - In the Matter of Anthony T. Rivera WBA-14-0006 - In the Matter of Anthony T. Rivera On March 9, 2015, OHA denied an Appeal of the dismissal of a complaint filed by Anthony T. Rivera (Rivera) against Lawrence Livermore National Security (LLNS), management and operating contractor for DOE's Lawrence Livermore National Laboratory, under the DOE's Contractor Employee Protection Program (10 CFR Part 708). In his complaint, Rivera alleges that he was terminated from his position with LLNS because

  14. WBA-15-0009 - In the Matter of Sandra Black | Department of Energy

    Energy Savers [EERE]

    9 - In the Matter of Sandra Black WBA-15-0009 - In the Matter of Sandra Black On December 31, 2015, OHA denied an Appeal involving a Complaint filed by Sandra Black against Savannah River Nuclear Solutions, LLC (SRNS) under the DOE's Contractor Employee Protection Program, 10 CFR Part 708. In her Complaint, Black alleged SRNS terminated her for engaging in protected activities, specifically citing her participation in a Government Accountability Office review as a protected disclosure. An OHA

  15. FIA-16-0039 - In the Matter of Michael Ravnitzky | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    9 - In the Matter of Michael Ravnitzky FIA-16-0039 - In the Matter of Michael Ravnitzky On July 28, 2016, OHA granted in part a FOIA Appeal filed by Michael Ravinitzky from a determination issued by the Office of Scientific and Technical Information (OSTI) of the Department of Energy. In the Appeal, the Appellant challenged OSTI's decision to withhold responsive records under Exemptions 3 and 4 of the FOIA. Reviewing only the unclassified portion of the responsive records, OHA found that OSTI's

  16. PSH-14-0109 - In the Matter of Personnel Security Hearing | Department of

    Energy Savers [EERE]

    Energy 109 - In the Matter of Personnel Security Hearing PSH-14-0109 - In the Matter of Personnel Security Hearing On May 11, 2015, an Administrative Judge issued a decision in which he concluded that an individual's security clearance should not be restored. OPM investigators discovered during a periodic reinvestigation of the individual that he had stolen money from a Sports Venue where he worked part-time (outside of the DOE complex). The individual acknowledged during an interview with

  17. PSH-16-0032 - In the Matter of Personnel Security Hearing | Department of

    Energy Savers [EERE]

    Energy 2 - In the Matter of Personnel Security Hearing PSH-16-0032 - In the Matter of Personnel Security Hearing On August 9, 2016, an Administrative Judge issued a decision in which she determined that an individual's access authorization should not be restored. In October 2015, as part of a background investigation, the Local Security Office (LSO) conducted a Personnel Security Interview (PSI) of the individual to address concerns about his falsifications and alcohol use. In addition to

  18. TEE-0012 - In the Matter of Electrolux Home Products, Inc. | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Energy 2 - In the Matter of Electrolux Home Products, Inc. TEE-0012 - In the Matter of Electrolux Home Products, Inc. This Decision and Order considers an Application for Exception filed by Electrolux Home Products, Inc. (EHP) seeking exception relief from the provisions of 10 C.F.R. Part 430, pertaining to energy conservation standards for refrigerators, refrigerator-freezers and freezers (Refrigerator Efficiency Standards). In its exception request, EHP asserts that the firm would suffer a

  19. TEE-0013 - In the Matter of NORDYNE, Inc. | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    3 - In the Matter of NORDYNE, Inc. TEE-0013 - In the Matter of NORDYNE, Inc. This Decision and Order considers an Application for Exception filed by NORDYNE, Inc. (NORDYNE), seeking exception relief from the provisions of 10 C.F.R. Part 430, pertaining to energy conservation standards for central air conditioners and heat pumps (Air Conditioner Standards). NORDYNE manufacturers air conditioning and heating equipment for the residential, light commercial and manufactured housing markets. In its

  20. TEE-0022 - In the Matter of Maytag Corporation | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    2 - In the Matter of Maytag Corporation TEE-0022 - In the Matter of Maytag Corporation This Decision and Order considers an Application for Exception filed by Maytag Corporation (Maytag) seeking exception relief from the provisions of 10 C.F.R. Part 430, Energy Conservation Program for Consumer Products: Energy Conservation Standards for Refrigerators, Refrigerator-Freezers and Freezers (Refrigerator Efficiency Standards). In its exception request, Maytag asserts that the firm would suffer a

  1. TEE-0025 - In the Matter of LG Electronics, Inc. | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    5 - In the Matter of LG Electronics, Inc. TEE-0025 - In the Matter of LG Electronics, Inc. This Decision and Order considers an Application for Exception filed by LG Electronics, Inc. (LG) seeking exception relief from the provisions of 10 C.F.R. Part 430, Energy Conservation Program for Consumer Products: Energy Conservation Standards for Refrigerators, Refrigerator-Freezers and Freezers (Refrigerator Efficiency Standards). In its exception request, LG asserts that the firm would suffer a gross

  2. TEE-0047 - In the Matter of Samsung Electronics America | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Energy 47 - In the Matter of Samsung Electronics America TEE-0047 - In the Matter of Samsung Electronics America This Decision and Order considers an Application for Exception filed by Samsung Electronics America (Samsung) seeking relief from the provisions of 10 C.F.R. Part 430, Energy Conservation Program for Consumer Products: Energy Conservation Standards for Refrigerators, Refrigerator-Freezers and Freezers (Refrigerator Efficiency Standards). In its exception request, Samsung asserts 1

  3. VBU-0039 - In the Matter of Edward J. Seawalt | Department of Energy

    Office of Environmental Management (EM)

    VBH-0062 - In the Matter of Sue Rice Gossett VBH-0062 - In the Matter of Sue Rice Gossett This Initial Agency Decision concerns a whistleblower complaint filed by Sue Rice Gossett (Gossett) against her former employer, the Safety and Ecology Corporation (SEC), under the Department of Energy's (DOE) Contractor Employee Protection Program, which is codified at 10 C.F.R. Part 708. SEC is a sub-contractor of Bechtel Jacobs Corporation (BJC), the DOE's Managing Contractor at the Portsmouth Site in

  4. VEE-0081 - In the Matter of North Side Coal & Oil Co., Inc. | Department of

    Office of Environmental Management (EM)

    62 - In the Matter of Sue Rice Gossett VBZ-0062 - In the Matter of Sue Rice Gossett This Initial Agency Decision concerns a whistleblower complaint filed by Sue Rice Gossett (Gossett) against her former employer, the Safety and Ecology Corporation (SEC), under the Department of Energy's (DOE) Contractor Employee Protection Program, which is codified at 10 C.F.R. Part 708. SEC is a sub-contractor of Bechtel Jacobs Corporation (BJC), the DOE's Managing Contractor at the Portsmouth Site in Piketon,

  5. WBU-13-0013 - In the Matter of Sabine Lauer | Department of Energy

    Office of Environmental Management (EM)

    4-0006 - In the Matter of Anthony T. Rivera WBA-14-0006 - In the Matter of Anthony T. Rivera On March 9, 2015, OHA denied an Appeal of the dismissal of a complaint filed by Anthony T. Rivera (Rivera) against Lawrence Livermore National Security (LLNS), management and operating contractor for DOE's Lawrence Livermore National Laboratory, under the DOE's Contractor Employee Protection Program (10 CFR Part 708). In his complaint, Rivera alleges that he was terminated from his position with LLNS

  6. WBU-14-0005 - In the Matter of Frank T. Clark | Department of Energy

    Office of Environmental Management (EM)

    5 - In the Matter of Frank T. Clark WBU-14-0005 - In the Matter of Frank T. Clark On November 14, 2013, the Office of Hearings and Appeals (OHA) issued a decision denying Mr. Frank T. Clark's (Clark) Appeal of the National Nuclear Security Administration Whistleblower Program Manager's (Manager) dismissal of his whistleblower complaint for failure to present an issue to which relief could be granted under Part 708. Mr. Clark's complaint alleged that, during the period 2008 to 2010, he was

  7. PSH-16-0008 - In the Matter of Personnel Security Hearing | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Energy 8 - In the Matter of Personnel Security Hearing PSH-16-0008 - In the Matter of Personnel Security Hearing On May 19, 2016, an Administrative Judge issued a decision in which she determined that an individual's access authorization should not be restored. In August 2015, as part of a background investigation, the Local Security Office (LSO) conducted a Personnel Security Interview (PSI) of the individual to address concerns about his alcohol-related arrests and alcohol use. In addition

  8. PSH-16-0012 - In the Matter of Personnel Security Hearing | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Energy 2 - In the Matter of Personnel Security Hearing PSH-16-0012 - In the Matter of Personnel Security Hearing On June 20, 2016, an Administrative Judge issued a decision in which she determined that an individual's access authorization should be granted. In October 2015, as part of a background investigation, the Local Security Office (LSO) conducted a Personnel Security Interview (PSI) of the individual to address concerns about his gambling. In addition to the PSI, the LSO requested the

  9. PSH-12-0121 - In the Matter of Personnel Security Hearing | Department of

    Office of Environmental Management (EM)

    Energy 21 - In the Matter of Personnel Security Hearing PSH-12-0121 - In the Matter of Personnel Security Hearing This Decision concerns the eligibility of XXXXXXXX (hereinafter referred to as "the individual") to hold an access authorization under the Department of Energy's (DOE) regulations set forth at 10 C.F.R. Part 710, Subpart A, entitled, "General Criteria and Procedures for Determining Eligibility for Access to Classified Matter or Special Nuclear Material." As

  10. TBZ-0003 - In the Matter of Gilbert J. Hinojos | Department of Energy

    Office of Environmental Management (EM)

    03 - In the Matter of Gilbert J. Hinojos TBZ-0003 - In the Matter of Gilbert J. Hinojos This determination will consider a Motion to Dismiss filed by Honeywell Federal Manufacturing & Technologies (Honeywell) on April 21, 2003. Honeywell seeks dismissal of the underlying complaint filed by Gilbert J. Hinojos under the Department of Energy's Contractor Employee Protection Program, 10 C.F.R. Part 708. tbz0003.pdf (14.56 KB) More Documents & Publications WBU-15-0007 - In the Matter of

  11. VBU-0050 - In the Matter of Darryl H. Shadel | Department of Energy

    Office of Environmental Management (EM)

    50 - In the Matter of Darryl H. Shadel VBU-0050 - In the Matter of Darryl H. Shadel Darryl H. Shadel (the complainant) appeals the dismissal of his whistleblower complaint under 10 C.F.R. Part 708, the DOE Contractor Employee Protection Program. As explained below, I have determined that the complaint was improperly dismissed, and that further processing should be accorded. vbu0050.pdf (20.54 KB) More Documents & Publications TBU-0047 - In the Matter of Dennis D. Patterson TBU-0040 - In the

  12. VBZ-0057 - In the Matter of Janet K. Benson | Department of Energy

    Office of Environmental Management (EM)

    7 - In the Matter of Janet K. Benson VBZ-0057 - In the Matter of Janet K. Benson This determination considers Motions to Dismiss(1) filed by Lawrence Livermore National Laboratory (Laboratory)(2) under the Department of Energy's (DOE's) Contractor Employee Protection Program, 10 C.F.R. Part 708. In these Motions, the Laboratory contends that the claims asserted by Janet Benson in OHA Case No. VWA-0044 are defective as a matter of law and should not be determined on the merits.(3) The Laboratory

  13. VBZ-0058 - In the Matter of Janet K. Benson | Department of Energy

    Office of Environmental Management (EM)

    8 - In the Matter of Janet K. Benson VBZ-0058 - In the Matter of Janet K. Benson This determination considers Motions to Dismiss(1) filed by Lawrence Livermore National Laboratory (Laboratory)(2) under the Department of Energy's (DOE's) Contractor Employee Protection Program, 10 C.F.R. Part 708. In these Motions, the Laboratory contends that the claims asserted by Janet Benson in OHA Case No. VWA-0044 are defective as a matter of law and should not be determined on the merits.(3) The Laboratory

  14. Geometry Matters | The Ames Laboratory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Geometry Matters Researchers have discovered how the geometry of gold nanoparticles affects their images. Gold nanoparticles can be imaged optically and their movements can be seen using a technique known as differential interference contrast (DIC) microscopy. How gold nanoparticles appear in these images depends upon their environment. This can be used to learn about time-dependent nanoscale processes. However, an outstanding question has been whether or not the geometry of the gold particles

  15. Scalar graviton as dark matter

    SciTech Connect (OSTI)

    Pirogov, Yu. F.

    2015-06-15

    The basics of the theory of unimodular bimode gravity built on the principles of unimodular gauge invariance/relativity and general covariance are exposed. Besides the massless tensor graviton of General Relativity, the theory includes an (almost) massless scalar graviton treated as the gravitational dark matter. A spherically symmetric vacuum solution describing the coherent scalar-graviton field for the soft-core dark halos, with the asymptotically flat rotation curves, is demonstrated as an example.

  16. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    G Contract No. DE-AC06-09RL14728 G-i PART I - THE SCHEDULE SECTION G CONTRACT ADMINISTRATION DATA TABLE OF CONTENTS G.1 CONTRACT ADMINISTRATION ......

  17. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    G Contract No. DE-AC27-08RV14800 Modification No. 020 G-i PART I - THE SCHEDULE SECTION G CONTRACT ADMINISTRATION DATA TABLE OF CONTENTS G.1 CONTRACT ADMINISTRATION...

  18. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    G Contract No. DE-AC06-08RL14788 G-i PART I - THE SCHEDULE SECTION G CONTRACT ADMINISTRATION DATA TABLE OF CONTENTS G.1 CONTRACT ADMINISTRATION ......

  19. _PART I - THE SCHEDULE

    National Nuclear Security Administration (NNSA)

    572 dated 3215 Contract No. DE-AC04-94AL85000 Modification No. M202 Page 2 Part I - The Schedule Sections B through H TABLE OF CONTENTS B-1 SERVICES BEING ACQUIRED...

  20. _Part II - Contract Clauses

    National Nuclear Security Administration (NNSA)

    M0572 dated 3215 Contract DE-AC04-94AL85000 Modification No. M202 Page I - 1 Part II - Contract Clauses Section I TABLE OF CONTENTS 1. FAR 52.202-1 DEFINITIONS (JAN 2012)...

  1. _PART I - THE SCHEDULE

    National Nuclear Security Administration (NNSA)

    93015 to Mod 0588 Contract No. DE-AC04-94AL85000 Modification No. M202 Page 2 Part I - The Schedule Sections B through H TABLE OF CONTENTS B-1 SERVICES BEING ACQUIRED...

  2. Effects of Advanced Combustion Technologies on Particulate Matter...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Advanced Combustion Technologies on Particulate Matter Emissions Characteristics Effects of Advanced Combustion Technologies on Particulate Matter Emissions Characteristics ...

  3. Dark Matter in the MSSM

    SciTech Connect (OSTI)

    Cotta, R.C.; Gainer, J.S.; Hewett, J.L.; Rizzo, T.G.; /SLAC

    2009-04-07

    We have recently examined a large number of points in the parameter space of the phenomenological MSSM, the 19-dimensional parameter space of the CP-conserving MSSM with Minimal Flavor Violation. We determined whether each of these points satisfied existing experimental and theoretical constraints. This analysis provides insight into general features of the MSSM without reference to a particular SUSY breaking scenario or any other assumptions at the GUT scale. This study opens up new possibilities for SUSY phenomenology both in colliders and in astrophysical experiments. Here we shall discuss the implications of this analysis relevant to the study of dark matter.

  4. FIA-15-0035 - In the Matter of the Center for Public Integrity and

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Alexander Cohen | Department of Energy 5 - In the Matter of the Center for Public Integrity and Alexander Cohen FIA-15-0035 - In the Matter of the Center for Public Integrity and Alexander Cohen On July 28, 2015, OHA denied in part and remanded in part a FOIA Appeal filed by the Center for Public Integrity and Mr. Alexander Cohen (Appellants). The Appeal related to a FOIA request filed by the Appellants seeking records on an investigation by the Office of Inspector General (OIG) regarding

  5. FIA-15-0058 - In the Matter of Bradley P. Jones | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    8 - In the Matter of Bradley P. Jones FIA-15-0058 - In the Matter of Bradley P. Jones On November 10, 2015, OHA granted in part and denied in part a FOIA and Privacy Act Appeal filed by Bradley P. Jones from a determination issued to him by the DOE Office of the Inspector General (OIG). In the Appeal, the Appellant challenged the use of Exemptions 5, 6, 7(A), 7(C), and 7(D) and the adequacy of the search for responsive documents. OHA found that although the use of the exemptions was appropriate,

  6. TBB-0049 - In the Matter of Gary S. Vander Boegh | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    TBB-0049 - In the Matter of Gary S. Vander Boegh TBB-0049 - In the Matter of Gary S. Vander Boegh This letter concerns the complaint of retaliation that you filed with the Department of Energy (DOE) under 10 C.F.R. Part 708. On September 6, 2006, the Office of Hearings and Appeals (OHA) received your petition for Secretarial review of the August 3 jurisdictional appeal decision issued by the OHA Director. Under the Part 708 regulations, the Secretary will reverse or revise an appeal decision by

  7. TBH-0042 - In the Matter of Curtis Hall | Department of Energy

    Office of Environmental Management (EM)

    TBB-0049 - In the Matter of Gary S. Vander Boegh TBB-0049 - In the Matter of Gary S. Vander Boegh This letter concerns the complaint of retaliation that you filed with the Department of Energy (DOE) under 10 C.F.R. Part 708. On September 6, 2006, the Office of Hearings and Appeals (OHA) received your petition for Secretarial review of the August 3 jurisdictional appeal decision issued by the OHA Director. Under the Part 708 regulations, the Secretary will reverse or revise an appeal decision by

  8. Flavored dark matter beyond minimal flavor violation

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Agrawal, Prateek; Blanke, Monika; Gemmler, Katrin

    2014-10-13

    We study the interplay of flavor and dark matter phenomenology for models of flavored dark matter interacting with quarks. We allow an arbitrary flavor structure in the coupling of dark matter with quarks. This coupling is assumed to be the only new source of violation of the Standard Model flavor symmetry extended by a U(3)x associated with the dark matter. We call this ansatz Dark Minimal Flavor Violation (DMFV) and highlight its various implications, including an unbroken discrete symmetry that can stabilize the dark matter. As an illustration we study a Dirac fermionic dark matter ? which transforms asmoretriplet under U(3)x , and is a singlet under the Standard Model. The dark matter couples to right-handed down-type quarks via a colored scalar mediator ? with a coupling ?. We identify a number of flavor-safe scenarios for the structure of ? which are beyond Minimal Flavor Violation. For dark matter and collider phenomenology we focus on the well-motivated case of b-flavored dark matter. The combined flavor and dark matter constraints on the parameter space of ? turn out to be interesting intersections of the individual ones. LHC constraints on simplified models of squarks and sbottoms can be adapted to our case, and monojet searches can be relevant if the spectrum is compressed.less

  9. Flavored dark matter beyond Minimal Flavor Violation

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Agrawal, Prateek; Blanke, Monika; Gemmler, Katrin

    2014-10-13

    We study the interplay of flavor and dark matter phenomenology for models of flavored dark matter interacting with quarks. We allow an arbitrary flavor structure in the coupling of dark matter with quarks. This coupling is assumed to be the only new source of violation of the Standard Model flavor symmetry extended by a U(3) χ associated with the dark matter. We call this ansatz Dark Minimal Flavor Violation (DMFV) and highlight its various implications, including an unbroken discrete symmetry that can stabilize the dark matter. As an illustration we study a Dirac fermionic dark matter χ which transforms asmore » triplet under U(3) χ , and is a singlet under the Standard Model. The dark matter couples to right-handed down-type quarks via a colored scalar mediator Φ with a coupling λ. We identify a number of “flavor-safe” scenarios for the structure of λ which are beyond Minimal Flavor Violation. Also, for dark matter and collider phenomenology we focus on the well-motivated case of b-flavored dark matter. Furthermore, the combined flavor and dark matter constraints on the parameter space of λ turn out to be interesting intersections of the individual ones. LHC constraints on simplified models of squarks and sbottoms can be adapted to our case, and monojet searches can be relevant if the spectrum is compressed.« less

  10. Flavored dark matter beyond Minimal Flavor Violation

    SciTech Connect (OSTI)

    Agrawal, Prateek; Blanke, Monika; Gemmler, Katrin

    2014-10-13

    We study the interplay of flavor and dark matter phenomenology for models of flavored dark matter interacting with quarks. We allow an arbitrary flavor structure in the coupling of dark matter with quarks. This coupling is assumed to be the only new source of violation of the Standard Model flavor symmetry extended by a U(3) χ associated with the dark matter. We call this ansatz Dark Minimal Flavor Violation (DMFV) and highlight its various implications, including an unbroken discrete symmetry that can stabilize the dark matter. As an illustration we study a Dirac fermionic dark matter χ which transforms as triplet under U(3) χ , and is a singlet under the Standard Model. The dark matter couples to right-handed down-type quarks via a colored scalar mediator Φ with a coupling λ. We identify a number of “flavor-safe” scenarios for the structure of λ which are beyond Minimal Flavor Violation. Also, for dark matter and collider phenomenology we focus on the well-motivated case of b-flavored dark matter. Furthermore, the combined flavor and dark matter constraints on the parameter space of λ turn out to be interesting intersections of the individual ones. LHC constraints on simplified models of squarks and sbottoms can be adapted to our case, and monojet searches can be relevant if the spectrum is compressed.

  11. How cold is cold dark matter?

    SciTech Connect (OSTI)

    Armendariz-Picon, Cristian; Neelakanta, Jayanth T. E-mail: jtneelak@syr.edu

    2014-03-01

    If cold dark matter consists of particles, these must be non-interacting and non-relativistic by definition. In most cold dark matter models however, dark matter particles inherit a non-vanishing velocity dispersion from interactions in the early universe, a velocity that redshifts with cosmic expansion but certainly remains non-zero. In this article, we place model-independent constraints on the dark matter temperature to mass ratio, whose square root determines the dark matter velocity dispersion. We only assume that dark matter particles decoupled kinetically while non-relativistic, when galactic scales had not entered the horizon yet, and that their momentum distribution has been Maxwellian since that time. Under these assumptions, using cosmic microwave background and matter power spectrum observations, we place upper limits on the temperature to mass ratio of cold dark matter today (away from collapsed structures). These limits imply that the present cold dark matter velocity dispersion has to be smaller than 54 m/s. Cold dark matter has to be quite cold, indeed.

  12. A Matter of Quantum Voltages

    SciTech Connect (OSTI)

    Sellner, Bernhard; Kathmann, Shawn M.

    2014-11-14

    Voltages inside matter are relevant to crystallization, materials science, biology, catalysis, and aqueous chemistry. Electron holography is able to measure the variation of voltages in matter and modern supercomputers allow the calculation of quantum voltages with practically unlimited spatial and temporal resolution of bulk systems. Of particular interest is the Mean Inner Potential (Vo) - the spatial average of these voltages. Voltages are very sensitive to the distribution of electrons and provide metrics to understand interactions in condensed phases. In the present study, we find excellent agreement with measurements of Vo for vitrified water and salt crystals and demonstrate the impact of covalent and ionic bonding as well as intermolecular/atomic interactions. Furthermore, we predict Vo as well as the fluctuations of these voltages in aqueous NaCl electrolytes and characterize the changes in their behavior as the resolution increases below the size of atoms. This work was supported by the U.S. Department of Energy, Office of Basic Energy Sciences, Division of Chemical Sciences, Geosciences & Biosciences. Pacific Northwest National Laboratory (PNNL) is a multiprogram national laboratory operated for DOE by Battelle. This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231.

  13. _PART I - THE SCHEDULE

    National Nuclear Security Administration (NNSA)

    B - H, Page i PART I - THE SCHEDULE TABLE OF CONTENTS SECTION B: SUPPLIES OR SERVICES AND PRICES/COSTS ......................................................................... 3 B-1 SERVICES BEING ACQUIRED ........................................................................................................ 3 CLIN 0001 MANAGEMENT AND OPERATION OF THE NEVADA NATIONAL SECURITY SITE ............. 3 CLIN 0001A TRANSITION TERM

  14. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    124 i PART I - THE SCHEDULE SECTION F - DELIVERIES OR PERFORMANCE TABLE OF CONTENTS F.1 PERIOD OF PERFORMANCE ....................................................................... 1 F.2 PRINCIPAL PLACE OF PERFORMANCE .................................................... 1 F.3 DELIVERIES .................................................................................................. 1 F.4 FAR 52.242-15 STOP-WORK ORDER (AUG 1989) - ALT 1 (APR 1989) ..... 1 F.5 STOP-WORK AND SHUTDOWN

  15. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Contract No. DE-AC27-10RV15051 Conformed Thru Contract Modification No. A001 i PART I - THE SCHEDULE SECTION E - INSPECTION AND ACCEPTANCE TABLE OF CONTENTS E.1 FAR 52.246-5 INSPECTION OF SERVICES - COST-REIMBURSEMENT (APR 1984) ................................................................................................ 1 E.2 ACCEPTANCE .......................................................................................... 1 E.3

  16. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Contract No. DE-AC27-10RV15051 Conformed thru Contract Modification No. 109 i PART I - THE SCHEDULE SECTION G CONTRACT ADMINISTRATION DATA TABLE OF CONTENTS G.1 CORRESPONDENCE PROCEDURES .................................................... 1 G.2 CONTRACT ADMINISTRATION .............................................................. 2 G.3 CONTRACTOR'S POINT OF CONTACT ................................................. 3 G.4 DOE CONTRACTING OFFICER'S REPRESENTATIVE ......................... 3 G.5

  17. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    D Contract No. DE-AC06-09RL14728 D-i PART I - THE SCHEDULE SECTION D PACKAGING AND MARKING TABLE OF CONTENTS D.1 PACKAGING ................................................................................................................ D-1 D.2 MARKING .................................................................................................................... D-1 D.3 SECURITY REQUIREMENTS ...................................................................................... D-1 Mission

  18. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    D Contract No. DE-AC27-08RV14800 D-i PART I - THE SCHEDULE SECTION D PACKAGING AND MARKING TABLE OF CONTENTS D.1 PACKAGING ................................................................................................................ D-1 D.2 MARKING .................................................................................................................... D-1 D.3 SECURITY REQUIREMENTS ...................................................................................... D-1 Tank

  19. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    F Contract No. DE-AC27-08RV14800 Modification No. A015 F-i PART I - THE SCHEDULE SECTION F DELIVERIES OR PERFORMANCE TABLE OF CONTENTS F.1 PERIOD OF PERFORMANCE ........................................................................................................ 1 F.2 PRINCIPAL PLACE OF PERFORMANCE ...................................................................................... 1 F.3 FAR 52.242-15, STOP-WORK ORDER (AUG 1989) -- ALTERNATE I (APR 1984) ...................... 2 Tank

  20. Ultrafast Spectroscopy of Warm Dense Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Ultrafast Spectroscopy of Warm Dense Matter Ultrafast Spectroscopy of Warm Dense Matter Print Wednesday, 25 April 2012 00:00 Being neither solid, liquid, gas, nor plasma, warm dense matter (WDM) occupies a no man's land in the map of material phases. Its temperature can range between that of planetary cores (tens of thousands K) to that of stellar cores (hundreds of thousands K). Not only is it prevalent throughout the universe, it is relevant to inertial confinement fusion (ICF) and material

  1. TASI 2008 Lectures on Dark Matter

    SciTech Connect (OSTI)

    Hooper, Dan; /Fermilab /Chicago U., Astron. Astrophys. Ctr.

    2009-01-01

    Based on lectures given at the 2008 Theoretical Advanced Study Institute (TASI), I review here some aspects of the phenomenology of particle dark matter, including the process of thermal freeze-out in the early universe, and the direct and indirect detection of WIMPs. I also describe some of the most popular particle candidates for dark matter and summarize the current status of the quest to discover dark matter's particle identity.

  2. Pump Systems Matter Mission and Vision:

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Pump Systems Matter Mission and Vision: Pump Systems Matter(tm) (PSM) places a primary focus on pump systems education and outreach and addresses energy savings and total cost of pump ownership. Vision: Pump Systems Matter initiative assists North American pump users gain a more competitive business advantage through strategic, broad-based energy management and pump system performance optimization. Mission: To provide the marketplace with tools and collaborative opportunities to integrate pump

  3. Complementarity of direct dark matter detection and indirect detection through gamma rays

    SciTech Connect (OSTI)

    Bergstroem, Lars; Bringmann, Torsten; Edsjoe, Joakim

    2011-02-15

    We show, by using an extensive sample of viable supersymmetric models as templates, that indirect detection of dark matter through gamma rays may have a large potential for identifying the nature of dark matter. This is, in particular, true also for models that give too weak dark matter-nucleon scattering cross sections to be probed by present and planned direct detection experiments. Also models with a mass scale too high to be accessible at CERN's LHC accelerator may show up in next-generation imaging Cherenkov telescope arrays. Based on our findings, we therefore suggest to view indirect searches as genuine particle physics experiments, complementing other strategies to probe so far unknown regions in the parameter space of e.g. supersymmetric models, and propose a new approach that would make use of telescopes dedicated for dark matter searches. As a concrete example for the potential of such an approach, we consider an array of imaging air Cherenkov telescopes, the Dark Matter Array (DMA), and show that such an experiment could extend present-day limits by several orders of magnitude, reaching a large class of models that would remain undetected in both direct detection experiments and searches at the LHC. In addition, in a sizable part of the parameter space, signals from more than one type of dark matter detection experiment would be possible, something that may eventually be necessary in order to identify the dark matter candidate.

  4. Neutrino signals from dark matter decay

    SciTech Connect (OSTI)

    Covi, Laura; Grefe, Michael; Ibarra, Alejandro; Tran, David E-mail: michael.grefe@desy.de E-mail: david.tran@ph.tum.de

    2010-04-01

    We investigate different neutrino signals from the decay of dark matter particles to determine the prospects for their detection, and more specifically if any spectral signature can be disentangled from the background in present and future neutrino observatories. If detected, such a signal could bring an independent confirmation of the dark matter interpretation of the dramatic rise in the positron fraction above 10 GeV recently observed by the PAMELA satellite experiment and offer the possibility of distinguishing between astrophysical sources and dark matter decay or annihilation. In combination with other signals, it may also be possible to distinguish among different dark matter decay channels.

  5. Astrophysical tests of mirror dark matter

    SciTech Connect (OSTI)

    Ciarcelluti, P.

    2008-08-29

    Mirror matter is a self-collisional dark matter candidate. If exact mirror parity is a conserved symmetry of the nature, there could exist a parallel hidden (mirror) sector of the Universe which has the same kind of particles and the same physical laws of our (visible) sector. The two sectors interact each other only via gravity, therefore mirror matter is naturally 'dark'. The most promising way to test this dark matter candidate is to look at its astrophysical signatures, as Big Bang nucleosynthesis, primordial structure formation and evolution, cosmic microwave background and large scale structure power spectra.

  6. Terra Matters PLLC | Open Energy Information

    Open Energy Info (EERE)

    to: navigation, search Name: Terra Matters, PLLC Place: Seattle, Washington Zip: 98122 Product: Boutique consultancy providing advice on sustainable design and business...

  7. Course Overview Pump Systems Matter Optimization | Department...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Course Overview Pump Systems Matter Optimization Attendees of the "Pump Systems Optimization" one-day course will gain valuable new skills to help them improve...

  8. ALS Reveals New State of Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    universe" of sorts. Some researchers believe that the conditions inside this new state of matter can be manipulated (for example, by bringing it into contact with a...

  9. Jelly Bean Universe (Dark Matter / Dark Energy)

    ScienceCinema (OSTI)

    Kurt Riesselmann

    2010-01-08

    Fermilab's Kurt Riesselmann explains how to make a jelly bean universe to help explain the mysteries of dark matter and dark energy.

  10. Ultrafast Spectroscopy of Warm Dense Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    the properties of all. In disciplines such as condensed matter or plasma physics, one force often dominates over the others, allowing smaller forces to be neglected in physical...

  11. Dipolar dark matter with massive bigravity

    SciTech Connect (OSTI)

    Blanchet, Luc; Heisenberg, Lavinia

    2015-12-14

    Massive gravity theories have been developed as viable IR modifications of gravity motivated by dark energy and the problem of the cosmological constant. On the other hand, modified gravity and modified dark matter theories were developed with the aim of solving the problems of standard cold dark matter at galactic scales. Here we propose to adapt the framework of ghost-free massive bigravity theories to reformulate the problem of dark matter at galactic scales. We investigate a promising alternative to dark matter called dipolar dark matter (DDM) in which two different species of dark matter are separately coupled to the two metrics of bigravity and are linked together by an internal vector field. We show that this model successfully reproduces the phenomenology of dark matter at galactic scales (i.e. MOND) as a result of a mechanism of gravitational polarisation. The model is safe in the gravitational sector, but because of the particular couplings of the matter fields and vector field to the metrics, a ghost in the decoupling limit is present in the dark matter sector. However, it might be possible to push the mass of the ghost beyond the strong coupling scale by an appropriate choice of the parameters of the model. Crucial questions to address in future work are the exact mass of the ghost, and the cosmological implications of the model.

  12. Jelly Bean Universe (Dark Matter / Dark Energy)

    SciTech Connect (OSTI)

    Kurt Riesselmann

    2009-09-10

    Fermilab's Kurt Riesselmann explains how to make a jelly bean universe to help explain the mysteries of dark matter and dark energy.

  13. Dark matter annihilation or unresolved astrophysical sources...

    Office of Scientific and Technical Information (OSTI)

    Citation Details In-Document Search Title: Dark matter annihilation or unresolved ... cosmic gamma-ray background (CGB) is a longstanding mystery in high-energy astrophysics. ...

  14. Dark matter in B-L extended MSSM models

    SciTech Connect (OSTI)

    Khalil, S.; Okada, H.

    2009-04-15

    We analyze the dark matter problem in the context of the supersymmetric U(1){sub B-L} model. In this model, the lightest neutralino can be the B-L gaugino Z-tilde{sub B-L} or the extra Higgsinos {chi}-tilde{sub 1,2} dominated. We compute the thermal relic abundance of these particles and show that, unlike the lightest neutralino in the MSSM, they can account for the observed relic abundance with no conflict with other phenomenological constraints. The prospects for their direct detection, if they are part of our galactic halo, are also discussed.

  15. Part III - Section J

    National Nuclear Security Administration (NNSA)

    Corporation Contract No. DE-AC04-94AL85000 Modification No. 585 Attachment 2 Page 1 of 5 Part III - Section J Appendix G List of Applicable Directives and NNSA Policy Letters In addition to the list of applicable directives referenced below, the contractor shall also comply with supplementary directives (e.g., manuals), which are invoked by a Contractor Requirements Document (CRD) attached to a directive referenced below. This List excludes directives that have been granted an exemption from the

  16. Part III - Section J

    National Nuclear Security Administration (NNSA)

    M280 Attachment 1 Page 1 of 5 Part III - Section J Appendix G List of Applicable Directives and NNSA Policy Letters In addition to the list of applicable directives referenced below, the contractor shall also comply with supplementary directives (e.g., manuals), which are invoked by a Contractor Requirements Document (CRD) attached to a directive referenced below. DIRECTIVE NUMBER DATE DOE DIRECTIVE TITLE APPH Chapter X Revision 10 09/08/98 Accounting Practices & Procedures Handbook Chapter

  17. _Part II - Contract Clauses

    National Nuclear Security Administration (NNSA)

    09/30/2015 to Mod 0588 Contract DE-AC04-94AL85000 Modification No. M202 Page I - 1 Part II - Contract Clauses Section I TABLE OF CONTENTS 1. FAR 52.202-1 DEFINITIONS (JAN 2012) (REPLACED M473) ............................................................. 8 2. FAR 52.203-3 GRATUITIES (APR 1984) ................................................................................................. 8 3. FAR 52.203-5 COVENANT AGAINST CONTINGENT FEES (APR 1984) ........................................... 9

  18. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    F Contract No. DE-AC06-09RL14728 Modification 343 PART I - THE SCHEDULE SECTION F DELIVERIES OR PERFORMANCE TABLE OF CONTENTS F.1 PERIOD OF PERFORMANCE .................................................................................... F-1 F.2 PRINCIPAL PLACE OF PERFORMANCE .................................................................. F-1 F.3 FAR 52.242-15, STOP-WORK ORDER (AUG 1989) - ALTERNATE I (APR 1984) ..... F-2 F-i Mission Support Contract Section F Contract No. DE-AC06-09RL14728

  19. PART I - THE SCHEDULE

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    E Contract No. DE-AC27-08RV14800 Modification No. A015 E-i PART I - THE SCHEDULE SECTION E INSPECTION AND ACCEPTANCE TABLE OF CONTENTS E.1 DOE INSPECTION AND ACCEPTANCE ........................................................................................... 1 E.2 FAR 52.246-3, INSPECTION OF SUPPLIES - COST-REIMBURSEMENT (MAY 2001) ................. 2 E.3 FAR 52.246-5, INSPECTION OF SERVICES - COST REIMBURSEMENT (APR 1984) ................. 3 Tank Operations Contract Section E Contract No.

  20. H5Part

    Energy Science and Technology Software Center (OSTI)

    2005-12-01

    Particle based simulations of accelerator beam-lines, especially in six dimensional phase space, generate vast amounts of data. Even though a subset of statistical information regarding phase space or analysis needs to be preserved, reading and writing such enormous restart files on massively parallel supercomputing systems remains challenging. H5Part is a very simple data storage schema and provides an API that simplifies the reading/writing of the data to the HDF5 file format. An important foundation formore » a stable visualization and data analysis environment is a stable and portable file storage format and its associated APIs. The presence of a "common file storage format," including associated APIs, will help foster a fundamental level of interoperability across the project’s software infrastructure. It will also haip ensure that key data analysis capabilities are present during the earliest phases of the software development effort. H5Part is built on top of the HDF5 (Hierarchical Data Format). HDF5 offers a self.describing machine-independent binary file format that supports scalable parallel I/O performance for MPI codes on a variety of supercomputlng systems, and works equally well on laptop computers. The API Is available (or C, C++, and Fortran codes. The H5Part file format and APIs enable disparate research groups with different simulation implementations to transparently share datasets and data analysis tools. For instance, the common file format will enable groups that depend on completely different simulation implementations to share data analysis tools like PartView and AVS/Express without any additional programming.« less

  1. Spin polarized asymmetric nuclear matter and neutron star matter within the lowest order constrained variational method

    SciTech Connect (OSTI)

    Bordbar, G. H.; Bigdeli, M.

    2008-01-15

    In this paper, we calculate properties of the spin polarized asymmetrical nuclear matter and neutron star matter, using the lowest order constrained variational (LOCV) method with the AV{sub 18}, Reid93, UV{sub 14}, and AV{sub 14} potentials. According to our results, the spontaneous phase transition to a ferromagnetic state in the asymmetrical nuclear matter as well as neutron star matter do not occur.

  2. Scientists Mix Matter and Anti-Matter Results to Resolve Decade-Old Proton

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Puzzle | Jefferson Lab Scientists Mix Matter and Anti-Matter Results to Resolve Decade-Old Proton Puzzle The CEBAF Large Acceptance Spectrometer, or CLAS, in Jefferson Lab's Experimental Hall B was used to measure electrons during the experiment. The CEBAF Large Acceptance Spectrometer, or CLAS, in Jefferson Lab's Experimental Hall B was used to measure electrons during the experiment. Scientists Mix Matter and Anti-Matter to Resolve Decade-Old Proton Puzzle Fans of science and science

  3. Hadronization line in stringy matter

    SciTech Connect (OSTI)

    Biro, Tamas S.; Cleymans, Jean

    2008-09-15

    The equation of state of the string model with linear strings comes close to describing the lattice quantum chromodynamics results and allows for the E/N{approx_equal}6T{sub 0}=1GeV relation found in phenomenological statistical model. The E/N value is derived from the zero pressure condition in quark matter and is a fairly general result. The baryochemical potential dependence of the hadron gas can be met if it is interpreted in the framework of an additive quark model. The conclusion is reached that stringy models explain the E/N=6T{sub 0} relation naturally and independently of the value of the string tension.

  4. Part B - Requirements & Funding Information PART B - Requirements...

    Office of Environmental Management (EM)

    IA, indicate whether Part A of the IA is attached or the location of Part A. For example, Part A could be located in the master file for IA number xxx at contracting office xxx. ...

  5. Part B - Requirements & Funding Information PART B - Requirements...

    Broader source: Energy.gov (indexed) [DOE]

    ... IA, indicate whether Part A of the IA is attached or the location of Part A. For example, Part A could be located in the master file for IA number xxx at contracting office xxx. ...

  6. Revisions to FAR Part 17 Special Contracting Methods and Part...

    Broader source: Energy.gov (indexed) [DOE]

    and Assistance Management SUBJECT: Revisions to FAR Part 17 Special Contracting Methods and Part 35 Research and Development Contracting SUMMARY: The Federal Register (77 FR...

  7. Decaying leptophilic dark matter at IceCube

    SciTech Connect (OSTI)

    Boucenna, Sofiane M.; Chianese, Marco; Mangano, Gianpiero; Miele, Gennaro; Morisi, Stefano; Pisanti, Ofelia; Vitagliano, Edoardo

    2015-12-29

    We present a novel interpretation of IceCube high energy neutrino events (with energy larger than 60 TeV) in terms of an extraterrestrial flux due to two different contributions: a flux originated by known astrophysical sources and dominating IceCube observations up to few hundreds TeV, and a new flux component where the most energetic neutrinos come from the leptophilic three-body decays of dark matter particles with a mass of few PeV. Differently from other approaches, we provide two examples of elementary particle models that do not require extremely tiny coupling constants. We find the compatibility of the theoretical predictions with the IceCube results when the astrophysical flux has a cutoff of the order of 100 TeV (broken power law). In this case the most energetic part of the spectrum (PeV neutrinos) is due to an extra component such as the decay of a very massive dark matter component. Due to the low statistics at our disposal we have considered for simplicity the equivalence between deposited and neutrino energy, however such approximation does not affect dramatically the qualitative results. Of course, a purely astrophysical origin of the neutrino flux (no cutoff in energy below the PeV scale — unbroken power law) is still allowed. If future data will confirm the presence of a sharp cutoff above few PeV this would be in favor of a dark matter interpretation.

  8. Advanced particulate matter control apparatus and methods

    DOE Patents [OSTI]

    Miller, Stanley J.; Zhuang, Ye; Almlie, Jay C.

    2012-01-10

    Apparatus and methods for collection and removal of particulate matter, including fine particulate matter, from a gas stream, comprising a unique combination of high collection efficiency and ultralow pressure drop across the filter. The apparatus and method utilize simultaneous electrostatic precipitation and membrane filtration of a particular pore size, wherein electrostatic collection and filtration occur on the same surface.

  9. _PART I - THE SCHEDULE

    National Nuclear Security Administration (NNSA)

    9/30/15 to Mod 0588 Contract No. DE-AC04-94AL85000 Modification No. M202 Page 2 Part I - The Schedule Sections B through H TABLE OF CONTENTS B-1 SERVICES BEING ACQUIRED ......................................................................................... 4 B-2 CONTRACT TYPE AND VALUE (Rev. M218, M222, M236, M241, M261, M266, M288, M293, M312, M319, M344, M365, M400, M404, M443, M448, M473, M484, M0512, M0528, M0538, M0541, M0563, M0567, A0588)

  10. PART II - CONTRACT CLAUSES

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    I Contract No. DE-AC06-09RL14728 Modification 479 I-1 PART II - CONTRACT CLAUSES SECTION I CONTRACT CLAUSES I.1 FAR 52.252-2 CLAUSES INCORPORATED BY REFERENCE (FEB 1998) This Contract incorporates one or more clauses by reference, with the same force and effect as if they were given in full text. Upon request, the Contracting Officer will make their full text available. Also, the full text of a clause may be accessed electronically at these addresses: https://www.acquisition.gov/far/index.html

  11. PART II - CONTRACT CLAUSES

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    I Contract No. DE-AC27-08RV14800 Modification No. 330 I-1 PART II - CONTRACT CLAUSES SECTION I CONTRACT CLAUSES I.1 FAR 52.252-2 CLAUSES INCORPORATED BY REFERENCE (FEB 1998) This Contract incorporates one or more clauses by reference, with the same force and effect as if they were given in full text. Upon request, the Contracting Officer will make their full text available. Also, the full text of a clause may be accessed electronically at these addresses: http://www.arnet.gov/far/

  12. Part A | Open Energy Information

    Open Energy Info (EERE)

    Document- Permit ApplicationPermit Application: Part ALegal Abstract RCRA Hazardous Waste Part A Permit Application, current through August 7, 2014. Published NA Year Signed...

  13. Ratcheting Up The Search for Dark Matter

    SciTech Connect (OSTI)

    McDermott, Samuel Dylan

    2014-01-01

    The last several years have included remarkable advances in two of the primary areas of fundamental particle physics: the search for dark matter and the discovery of the Higgs boson. This dissertation will highlight some contributions made on the forefront of these exciting fields. Although the circumstantial evidence supporting the dark matter hypothesis is now almost undeniably significant, indisputable direct proof is still lacking. As the direct searches for dark matter continue, we can maximize our prospects of discovery by using theoretical techniques complementary to the observational searches to rule out additional, otherwise accessible parameter space. In this dissertation, I report bounds on a wide range of dark matter theories. The models considered here cover the spectrum from the canonical case of self-conjugate dark matter with weak-scale interactions, to electrically charged dark matter, to non-annihilating, non-fermionic dark matter. These bounds are obtained from considerations of astrophysical and cosmological data, including, respectively: diffuse gamma ray photon observations; structure formation considerations, along with an explication of the novel local dark matter structure due to galactic astrophysics; and the existence of old pulsars in dark-matter-rich environments. I also consider the prospects for a model of neutrino dark matter which has been motivated by a wide set of seemingly contradictory experimental results. In addition, I include a study that provides the tools to begin solving the speculative ``inverse'' problem of extracting dark matter properties solely from hypothetical nuclear energy spectra, which we may face if dark matter is discovered with multiple direct detection experiments. In contrast to the null searches for dark matter, we have the example of the recent discovery of the Higgs boson. The Higgs boson is the first fundamental scalar particle ever observed, and precision measurements of the production and decay of

  14. Supersymmetric Dark Matter after LHC Run 1

    SciTech Connect (OSTI)

    Bagnaschi, E. A.; Buchmueller, O.; Cavanaugh, R.; Citron, M.; De Roeck, A.; Dolan, M. J.; Ellis, J. R.; Flacher, H.; Heinemeyer, S.; Isidori, G.; Malik, S.; Santos, D. Martinez; Olive, K. A.; Sakurai, K.; de Vries, K. J.; Weiglein, G.

    2015-10-23

    Different mechanisms operate in various regions of the MSSM parameter space to bring the relic density of the lightest neutralino, χ~01, assumed here to be the lightest SUSY particle (LSP) and thus the dark matter (DM) particle, into the range allowed by astrophysics and cosmology. These mechanisms include coannihilation with some nearly degenerate next-to-lightest supersymmetric particle such as the lighter stau τ~1, stop t~1 or chargino χ1, resonant annihilation via direct-channel heavy Higgs bosons H / A, the light Higgs boson h or the Z boson, and enhanced annihilation via a larger Higgsino component of the LSP in the focus-point region. These mechanisms typically select lower-dimensional subspaces in MSSM scenarios such as the CMSSM, NUHM1, NUHM2, and pMSSM10. We analyze how future LHC and direct DM searches can complement each other in the exploration of the different DM mechanisms within these scenarios. We find that the τ~1 coannihilation regions of the CMSSM, NUHM1, NUHM2 can largely be explored at the LHC via searches for /ET events and long-lived charged particles, whereas theirH / A funnel, focus-point and χ1 coannihilation regions can largely be explored by the LZ and Darwin DM direct detection experiments. Furthermore, we find that the dominant DM mechanism in our pMSSM10 analysis is χ~±1 coannihilation: parts of its parameter space can be explored by the LHC, and a larger portion by future direct DM searches.

  15. Supersymmetric Dark Matter after LHC Run 1

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Bagnaschi, E. A.; Buchmueller, O.; Cavanaugh, R.; Citron, M.; De Roeck, A.; Dolan, M. J.; Ellis, J. R.; Flacher, H.; Heinemeyer, S.; Isidori, G.; et al

    2015-10-23

    Different mechanisms operate in various regions of the MSSM parameter space to bring the relic density of the lightest neutralino, χ~01, assumed here to be the lightest SUSY particle (LSP) and thus the dark matter (DM) particle, into the range allowed by astrophysics and cosmology. These mechanisms include coannihilation with some nearly degenerate next-to-lightest supersymmetric particle such as the lighter stau τ~1, stop t~1 or chargino χ~±1, resonant annihilation via direct-channel heavy Higgs bosons H / A, the light Higgs boson h or the Z boson, and enhanced annihilation via a larger Higgsino component of the LSP in the focus-pointmore » region. These mechanisms typically select lower-dimensional subspaces in MSSM scenarios such as the CMSSM, NUHM1, NUHM2, and pMSSM10. We analyze how future LHC and direct DM searches can complement each other in the exploration of the different DM mechanisms within these scenarios. We find that the τ~1 coannihilation regions of the CMSSM, NUHM1, NUHM2 can largely be explored at the LHC via searches for /ET events and long-lived charged particles, whereas theirH / A funnel, focus-point and χ~±1 coannihilation regions can largely be explored by the LZ and Darwin DM direct detection experiments. Furthermore, we find that the dominant DM mechanism in our pMSSM10 analysis is χ~±1 coannihilation: parts of its parameter space can be explored by the LHC, and a larger portion by future direct DM searches.« less

  16. Nuclear and neutron matter studies

    SciTech Connect (OSTI)

    Wiringa, R.B.; Akmal, A.; Pandharipande, V.R.

    1995-08-01

    We are studying nuclear and neutron matter with the new Argonne v{sub 18} NN and Urbana 3N potentials. We use variational wave functions and a diagrammatic cluster expansion with Fermi hypernetted and single-operator chain (FHNC/SOC) integral equations to evaluate the energy expectation value. Initial results show some interesting differences with our previous calculations with the older Argonne v{sub 14} potential. In particular, there are a number of diagrams involving L{center_dot}S and L{sup 2} terms which were small with the older model and were rather crudely estimated or even neglected. It appears that these terms are more important with the new potential and will have to be evaluated more accurately. Work on this subject is in progress. A simple line of attack is to just add additional diagrams at the three-body cluster level. A longer term approach may be to adapt some of the methods for evaluating nucleon clusters used in the few-body and closed shell nuclei described above.

  17. Science on the Hill: Why space weather matters

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Why space weather matters Why space weather matters Many people think of space as a ... Science on the Hill: Why space weather matters Many people think of space as a silent, ...

  18. TBU-0119 - In the Matter of Gennady Ozeryansky | Department of...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    PDF icon tbu0119.pdf More Documents & Publications TBU-0113 - In the Matter of Gennady Ozeryansky TBB-0119 In the Matter of Gennady Ozeryansky TBU-0117 - In the Matter of Gordon ...

  19. Overview of Pump Systems Matter | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Overview of Pump Systems Matter Overview of Pump Systems Matter Pump Systems Matter (PSM) is a non-profit (501(c) 3) educational foundation, established to educate the marketplace and promote pumping systems energy efficiency. G_Overview_of_Pump_Systems_Matter.pdf (1.04 MB) More Documents & Publications Summary of 2011 Accomplishments HI & PSM Course Overview Pump Systems Matter Optimization Pump Systems Matter Mission and Vision

  20. Pump Systems Matter Mission and Vision | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Pump Systems Matter Mission and Vision Pump Systems Matter Mission and Vision Pump Systems Matter(tm) (PSM) places a primary focus on pump systems education and outreach and addresses energy savings and total cost of pump ownership. C_Vision_&_Mission_of_Pump_Systems_Matter.pdf (56.49 KB) More Documents & Publications Overview of Pump Systems Matter Hydraulic Institute Member Benefits Course Overview Pump Systems Matter Optimization

  1. Quintessence with quadratic coupling to dark matter

    SciTech Connect (OSTI)

    Boehmer, Christian G.; Chan, Nyein; Caldera-Cabral, Gabriela; Lazkoz, Ruth; Maartens, Roy

    2010-04-15

    We introduce a new form of coupling between dark energy and dark matter that is quadratic in their energy densities. Then we investigate the background dynamics when dark energy is in the form of exponential quintessence. The three types of quadratic coupling all admit late-time accelerating critical points, but these are not scaling solutions. We also show that two types of coupling allow for a suitable matter era at early times and acceleration at late times, while the third type of coupling does not admit a suitable matter era.

  2. ALS Reveals New State of Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    ALS Reveals New State of Matter ALS Reveals New State of Matter Print Wednesday, 13 October 2010 00:00 ALS user groups from Princeton and Stanford have been making waves this past year with several high-profile papers and extensive news coverage of their work on a new state of matter embodied by "topological insulators," materials that conduct electricity only on their surfaces. First identified at the ALS in 2007 by a Princeton team led by M. Zahid Hasan, topological insulators have

  3. MPA Materials Matter September 2014 (Technical Report) | SciTech...

    Office of Scientific and Technical Information (OSTI)

    MPA Materials Matter September 2014 Citation Details In-Document Search Title: MPA Materials Matter September 2014 You are accessing a document from the Department of Energy's...

  4. Properties of nuclear matter within the JISP16NNinteraction ...

    Office of Scientific and Technical Information (OSTI)

    Properties of nuclear matter within the JISP16NNinteraction Citation Details In-Document Search Title: Properties of nuclear matter within the JISP16NNinteraction Authors:...

  5. The Effective Field Theory of Dark Matter Direct Detection (Journal...

    Office of Scientific and Technical Information (OSTI)

    Effective Field Theory of Dark Matter Direct Detection Citation Details In-Document Search Title: The Effective Field Theory of Dark Matter Direct Detection You are accessing a...

  6. MPA Materials Matter January 2015 (Technical Report) | SciTech...

    Office of Scientific and Technical Information (OSTI)

    MPA Materials Matter January 2015 Citation Details In-Document Search Title: MPA Materials Matter January 2015 You are accessing a document from the Department of Energy's (DOE) ...

  7. MPA Materials Matter December 2015 (Technical Report) | SciTech...

    Office of Scientific and Technical Information (OSTI)

    MPA Materials Matter December 2015 Citation Details In-Document Search Title: MPA Materials Matter December 2015 You are accessing a document from the Department of Energy's ...

  8. Social Media and Messages that Matter - Top Tips and Tools |...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Social Media and Messages that Matter - Top Tips and Tools Social Media and Messages that Matter - Top Tips and Tools Better Buildings Residential Network Peer Exchange Call ...

  9. Sandia Energy - Control of Strong Light-Matter Coupling Using...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Control of Strong Light-Matter Coupling Using the Capacitance of Metamaterial Nanocavities Home Highlights - Energy Research Control of Strong Light-Matter Coupling Using the...

  10. An Effective Theory of Dirac Dark Matter (Journal Article) |...

    Office of Scientific and Technical Information (OSTI)

    Journal Article: An Effective Theory of Dirac Dark Matter Citation Details In-Document Search Title: An Effective Theory of Dirac Dark Matter A stable Dirac fermion with ...

  11. MPA Materials Matter December 2014 (Technical Report) | SciTech...

    Office of Scientific and Technical Information (OSTI)

    Technical Report: MPA Materials Matter December 2014 Citation Details In-Document Search Title: MPA Materials Matter December 2014 You are accessing a document from the ...

  12. Detecting electron neutrinos from solar dark matter annihilation...

    Office of Scientific and Technical Information (OSTI)

    Detecting electron neutrinos from solar dark matter annihilation by JUNO Citation Details In-Document Search Title: Detecting electron neutrinos from solar dark matter annihilation ...

  13. Precision Determination Of The Nonlinear Matter Power Spectrum...

    Office of Scientific and Technical Information (OSTI)

    Precision Determination Of The Nonlinear Matter Power Spectrum Citation Details In-Document Search Title: Precision Determination Of The Nonlinear Matter Power Spectrum You are...

  14. Electronic Structure of Warm Dense Matter via Multicenter Green...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Electronic Structure of Warm Dense Matter via Multicenter Green's Function Technique Research Personnel Modeling The proposed research addresses the Warm Dense Matter area...

  15. In the OSTI Collections: Dark Matter and Dark Energy | OSTI,...

    Office of Scientific and Technical Information (OSTI)

    Dark Matter and Dark Energy Recent observations of the universe, combined with Einstein's ... consists of entities very different from the matter and energy long familiar to us. ...

  16. Indirect detection of self-interacting asymmetric dark matter...

    Office of Scientific and Technical Information (OSTI)

    Indirect detection of self-interacting asymmetric dark matter Prev Next Title: Indirect detection of self-interacting asymmetric dark matter Authors: Pearce, Lauren ; ...

  17. Postinflationary Higgs Relaxation and the Origin of Matter-Antimatter...

    Office of Scientific and Technical Information (OSTI)

    Postinflationary Higgs Relaxation and the Origin of Matter-Antimatter Asymmetry Prev Next Title: Postinflationary Higgs Relaxation and the Origin of Matter-Antimatter ...

  18. VBA-0062 - In the Matter of Susan Rice Gossett | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    VBA-0062 - In the Matter of Susan Rice Gossett VBA-0062 - In the Matter of Susan Rice Gossett This Decision considers an Appeal of an Initial Agency Decision (IAD) issued on May 8, 2002, involving a Complaint filed by Susan Rice Gossett (Gossett or the Complainant) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. In her Complaint, Gossett claims that her former employer, the Safety and Ecology Company (SEC) terminated her as a retaliation for

  19. WBH-13-0017 - In the Matter of Edward G. Gallrein, III | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Energy WBH-13-0017 - In the Matter of Edward G. Gallrein, III WBH-13-0017 - In the Matter of Edward G. Gallrein, III On April 10, 2014, the Office of Hearings and Appeals (OHA) issued a decision granting two motions to dismiss the Part 708 Complaint filed by Edward G. Gallrein, III. Babcock & Wilcox Y-12, LLC, and GemTech Y-12, LLC, each filed a motion to dismiss Mr. Gallrein's Complaint against them, in which he alleged that he made disclosures protected under 10 C.F.R. § 708.5(a) that

  20. WBZ-13-0017 - In the Matter of Edward G. Gallrein, III | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Energy WBZ-13-0017 - In the Matter of Edward G. Gallrein, III WBZ-13-0017 - In the Matter of Edward G. Gallrein, III On April 10, 2014, the Office of Hearings and Appeals (OHA) issued a decision granting two motions to dismiss the Part 708 Complaint filed by Edward G. Gallrein, III. Babcock & Wilcox Y-12, LLC, and GemTech Y-12, LLC, each filed a motion to dismiss Mr. Gallrein's Complaint against them, in which he alleged that he made disclosures protected under 10 C.F.R. § 708.5(a) that

  1. WBU-16-0004 - In the Matter of Richard Lusby | Department of Energy

    Energy Savers [EERE]

    4 - In the Matter of Richard Lusby WBU-16-0004 - In the Matter of Richard Lusby On May 16, 2016, OHA denied an Appeal of a dismissal of a Complaint filed by Richard Lusby against Savannah River Nuclear Solutions (SRNS) under the Department of Energy's (DOE) Contractor Employee Protection Program, 10 CFR Part 708. In his Complaint, Mr. Lusby alleged that SRNS had failed to hire him for several positions for which he had applied. He further alleged that the contractor's actions constituted

  2. WBU-16-0006 - In the Matter Dr. Shou-Yuan Zhang | Department of Energy

    Energy Savers [EERE]

    6 - In the Matter Dr. Shou-Yuan Zhang WBU-16-0006 - In the Matter Dr. Shou-Yuan Zhang On July 14, 2016, OHA granted an Appeal involving a Complaint filed by Dr. Shou-Yuan Zhang against Brookhaven Science Associates (BSA) under the DOE's Contractor Employee Protection Program, 10 CFR Part 708. In his Complaint, Dr. Zhang alleged that in an email to a BSA official, he reported research misconduct and that, in response, BSA transferred him to a new position. The DOE's Brookhaven Site Office (BHSO)

  3. WBU-16-0007 - In the Matter of Charles Dalton | Department of Energy

    Energy Savers [EERE]

    7 - In the Matter of Charles Dalton WBU-16-0007 - In the Matter of Charles Dalton On August 12, 2016, OHA granted an Appeal of a dismissal of a Complaint filed by Mr. Charles Dalton against BWX Technologies, Inc. (BWXT) under the DOE's Contractor Employee Protection Program, 10 CFR Part 708. In his Complaint, Mr. Dalton alleged that he reported to the Nuclear Regulatory Commission (NRC) and the DOE's Inspector General (IG) various problems with the techniques used by BWXT to inspect the fuel

  4. AFV-14-0001 - In the Matter of Washington State Fleet Operations |

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Department of Energy AFV-14-0001 - In the Matter of Washington State Fleet Operations AFV-14-0001 - In the Matter of Washington State Fleet Operations On December 18, 2014, the Director of the Office of Hearings and Appeals issued a decision in which he denied 's Washington State Fleet Operations (Washington) Appeal of a determination issued on November 10, 2014, Alternative Fuel Transportation Program (AFTP) of the Department of Energy (DOE), under the provisions of 10 C.F.R. Part 490. In

  5. TBH-0027 - In the Matter of Clint Olson | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    27 - In the Matter of Clint Olson TBH-0027 - In the Matter of Clint Olson This Initial Agency Decision involves a whistleblower complaint filed by Mr. Clint Olson (also referred to as the complainant or the individual) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. The complainant is an employee of BWXT Pantex (BWXT), the Management and Operations Contractor at the DOE's Pantex Plant in Amarillo, Texas. From July 1999 until November 2004, he was

  6. TBH-0047 - In the Matter of Dennis Patterson | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    47 - In the Matter of Dennis Patterson TBH-0047 - In the Matter of Dennis Patterson This Initial Agency Decision involves a whistleblower complaint filed by Mr. Dennis Patterson ("Patterson," "the complainant," or "Complainant") under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. The complainant was an employee of Batelle Energy Alliance, LLC, ("BEA" or "the contractor") the management and operating

  7. TBH-0075 - In the Matter of Richard L. Rieckenberg | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    75 - In the Matter of Richard L. Rieckenberg TBH-0075 - In the Matter of Richard L. Rieckenberg This Initial Agency Decision involves two whistleblower complaints, one filed by Jonathan K. Strausbaugh (Case No. TBH-0073) and the other filed by Richard L. Rieckenberg (Case No. TBH-0075) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. Both complainants were employees of KSL Services, Inc. ("KSL" or "the contractor"), a contractor

  8. TEA-0012 - In the Matter of Commonwealth of Massachusetts | Department of

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Energy 2 - In the Matter of Commonwealth of Massachusetts TEA-0012 - In the Matter of Commonwealth of Massachusetts This Decision and Order considers an Appeal filed by the Commonwealth of Massachusetts ("Massachusetts" or "the Commonwealth") from a determination issued on September 3, 2009, on behalf of the Assistant Secretary for Energy Efficiency and Renewable Energy (EE) of the Department of Energy (DOE), under the provisions of 10 C.F.R. Part 490 (Alternative Fuel

  9. TEA-0013 - In the Matter of Madison Gas and Electric Company | Department

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    of Energy 3 - In the Matter of Madison Gas and Electric Company TEA-0013 - In the Matter of Madison Gas and Electric Company This Decision and Order considers an Appeal filed by the Madison Gas and Electric Company (MGE) from a determination issued on September 17, 2009, on behalf of the Assistant Secretary for Energy Efficiency and Renewable Energy (EE) of the Department of Energy (DOE), under the provisions of 10 C.F.R. Part 490. In its determination, EE denied a request filed by MGE for

  10. TBA-0042 - In the Matter of Curtis Hall | Department of Energy

    Office of Environmental Management (EM)

    42 - In the Matter of Curtis Hall TBA-0042 - In the Matter of Curtis Hall This Decision considers two Appeals of an Initial Agency Decision (IAD) issued on March 15, 2007, by a Hearing Officer in the Department of Energy's (DOE) Office of Hearings and Appeals (OHA). The IAD addressed the merits of a whistleblower complaint filed by Curtis Hall against his former employer, Bechtel National, Inc. (BNI), under the Department of Energy's Contractor Employee Protection Program, 10 C.F.R. Part 708.

  11. TBA-0088 - In the Matter of Arun K. Dutta | Department of Energy

    Office of Environmental Management (EM)

    88 - In the Matter of Arun K. Dutta TBA-0088 - In the Matter of Arun K. Dutta This Decision considers an Appeal of an Initial Agency Decision (IAD) issued on August 25, 2010, involving a Complaint of Retaliation filed by Arun K. Dutta (Mr. Dutta or the complainant) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. In his Complaint, Mr. Dutta alleged that his former employer, Parsons Infrastructure and Technology Group, Inc. (Parsons or the

  12. TBH-0063 - In the Matter of Richard L. Urie | Department of Energy

    Office of Environmental Management (EM)

    7 - In the Matter of Dennis Patterson TBH-0047 - In the Matter of Dennis Patterson This Initial Agency Decision involves a whistleblower complaint filed by Mr. Dennis Patterson ("Patterson," "the complainant," or "Complainant") under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. The complainant was an employee of Batelle Energy Alliance, LLC, ("BEA" or "the contractor") the management and operating

  13. TBH-0089 - In the Matter of Himadri K. Das | Department of Energy

    Office of Environmental Management (EM)

    75 - In the Matter of Richard L. Rieckenberg TBH-0075 - In the Matter of Richard L. Rieckenberg This Initial Agency Decision involves two whistleblower complaints, one filed by Jonathan K. Strausbaugh (Case No. TBH-0073) and the other filed by Richard L. Rieckenberg (Case No. TBH-0075) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. Both complainants were employees of KSL Services, Inc. ("KSL" or "the contractor"), a contractor

  14. TBH-0096 - In the Matter of Douglas L. Cartledge | Department of Energy

    Office of Environmental Management (EM)

    96 - In the Matter of Douglas L. Cartledge TBH-0096 - In the Matter of Douglas L. Cartledge This Initial Agency Decision involves a whistleblower complaint filed by Douglas L. Cartledge ("Cartledge" or "the Complainant") under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. The Complainant was an employee of Parsons Corporation ("Parsons" or "the Contractor"), a first-tier contractor at the DOE Savannah River Site

  15. TBR-0112 - In the Matter of Ricky Ladd | Department of Energy

    Office of Environmental Management (EM)

    TBR-0112 - In the Matter of Ricky Ladd TBR-0112 - In the Matter of Ricky Ladd In a letter dated January 18, 2011, the Office of Hearings and Appeals (OHA) of the Department of Energy (DOE) dismissed the appeal of Ricky Ladd (hereinafter Mr. Ladd or the complainant) from the dismissal of his complaint of retaliation and request for investigation filed under 10 C.F.R. Part 708, the DOE Contractor Employee Protection Program (Case No. TBU-0112). After reconsidering Mr. Ladd's appeal in light of

  16. TBU-0071 - In the Matter of Jeffrey R. Burnette | Department of Energy

    Office of Environmental Management (EM)

    71 - In the Matter of Jeffrey R. Burnette TBU-0071 - In the Matter of Jeffrey R. Burnette Jeffrey R. Burnette (Burnette or the complainant), appeals the dismissal of his complaint of retaliation filed under 10 C.F.R. Part 708, the Department of Energy (DOE) Contractor Employee Protection Program. The complaint was dismissed for lack of jurisdiction under Section 708.17. As explained below, the dismissal of the complaint should be sustained, and the appeal denied. tbu0071.pdf (26.38 KB) More

  17. TBU-0081 - In the Matter of Leslie D. Cumiford | Department of Energy

    Office of Environmental Management (EM)

    81 - In the Matter of Leslie D. Cumiford TBU-0081 - In the Matter of Leslie D. Cumiford Leslie D. Cumiford ("the Complainant"), appeals the dismissal of her complaint of retaliation filed under 10 C.F.R. Part 708, the Department of Energy ("DOE") Contractor Employee Protection Program. The complaint was filed on October 10, 2006, and was dismissed on August 12, 2008. As explained below, the dismissal of the complaint should be affirmed, and the appeal denied. tbu0081.pdf

  18. TBZ-0063 - In the Matter of Richard L. Urie | Department of Energy

    Office of Environmental Management (EM)

    63 - In the Matter of Richard L. Urie TBZ-0063 - In the Matter of Richard L. Urie This Decision concerns a Complaint filed by Richard L. Urie (hereinafter referred to as "Mr. Urie" or "the Complainant") against Los Alamos National Laboratory (hereinafter referred to as "LANL" or "the Respondent"), his former employer, under the Department of Energy's (DOE) Contractor Employee Protection Program regulations found at 10 C.F.R. Part 708. At all times relevant

  19. TBZ-0104 In the Matter of Hansford F. Johnson | Department of Energy

    Office of Environmental Management (EM)

    104 In the Matter of Hansford F. Johnson TBZ-0104 In the Matter of Hansford F. Johnson This Decision will consider a Motion to Dismiss filed by B&W Pantex LLC (B&W), the Management and Operating Contractor for the Department of Energy's (DOE) Pantex Plant (Pantex), in connection with the pending Complaint of Retaliation filed by Hansford F. Johnson against B&W under the DOE's Contractor Employee Protection Program and its governing regulations set forth at 10 C.F.R. Part 708. The

  20. VBA-0082 - In the Matter of Janet K. Benson | Department of Energy

    Office of Environmental Management (EM)

    62 - In the Matter of Susan Rice Gossett VBA-0062 - In the Matter of Susan Rice Gossett This Decision considers an Appeal of an Initial Agency Decision (IAD) issued on May 8, 2002, involving a Complaint filed by Susan Rice Gossett (Gossett or the Complainant) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. In her Complaint, Gossett claims that her former employer, the Safety and Ecology Company (SEC) terminated her as a retaliation for making

  1. Hyperon-Nucleon Interactions and the Composition of Dense Matter from Quantum Chromodynamics

    SciTech Connect (OSTI)

    Konstantinos Orginos, Silas Beane, Emmanuel Chang, Saul Cohen, Huey-Wen Lin, Tom Luu, Assumpta Parreno, Martin Savage, Andre Walker-Loud, William Detmold

    2012-10-01

    The low-energy n{Sigma}{sup -} interactions determine, in part, the role of the strange quark in dense matter, such as that found in astrophysical environments. The scattering phase-shifts for this system are determined from a numerical evaluation of the QCD path integral using the technique of Lattice QCD. Our results, performed at a pion mass of m{sub {pi}} ~ 389 MeV in two large lattice volumes, and at one lattice spacing, are extrapolated to the physical pion mass using effective field theory. The calculated interactions indicate that the strange quark plays an important role in dense matter.

  2. Exploring the Nature of Matter | Jefferson Lab

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    of matter." And you might ask, what do they mean? At Jefferson Laboratory, we scatter electrons like Hofstadter did in the '50s when he explored nuclei. That's why one of our roads...

  3. Investigation of Direct Injection Vehicle Particulate Matter...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    This study focuses primarily on particulate matter mass analysis of a gasoline direct injection engine in a test cell with a chassis dynamometer. PDF icon p-10gibbs.pdf More ...

  4. Manual for Classified Matter Protection and Control

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    1998-01-09

    Provides detailed requirements for the protection and control of classified matter which supplement DOE O 471.2A. Cancels DOE M 471.2-1 dated 09/26/1995.

  5. Supernova cooling in a dark matter smog

    SciTech Connect (OSTI)

    Zhang, Yue

    2014-11-27

    A light hidden gauge boson with kinetic mixing with the usual photon is a popular setup in theories of dark matter. The supernova cooling via radiating the hidden boson is known to put an important constraint on the mixing. I consider the possible role dark matter, which under reasonable assumptions naturally exists inside supernova, can play in the cooling picture. Because the interaction between the hidden gauge boson and DM is likely unsuppressed, even a small number of dark matter compared to protons inside the supernova could dramatically shorten the free streaming length of the hidden boson. A picture of a dark matter “smog” inside the supernova, which substantially relaxes the cooling constraint, is discussed in detail.

  6. DOL: Role in EEOICPA – Part B and Part E

    Broader source: Energy.gov [DOE]

    DOL is tasked with administering the EEOICPA, both Parts B and E. Part B covers current and former workers who have been diagnosed with cancer, chronic beryllium disease, beryllium sensitivity, or...

  7. Ultrafast Spectroscopy of Warm Dense Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Spectroscopy of Warm Dense Matter Print Being neither solid, liquid, gas, nor plasma, warm dense matter (WDM) occupies a no man's land in the map of material phases. Its temperature can range between that of planetary cores (tens of thousands K) to that of stellar cores (hundreds of thousands K). Not only is it prevalent throughout the universe, it is relevant to inertial confinement fusion (ICF) and material performance under extreme conditions. However, because of its extreme temperatures and

  8. Light mixed sneutrinos as thermal dark matter

    SciTech Connect (OSTI)

    Bélanger, G.; Kakizaki, M.; Park, E.K.; Kraml, S.

    2010-11-01

    In supersymmetric models with Dirac neutrino masses, a left-right mixed sneutrino can be a viable dark matter candidate. We examine the MSSM+ν-tilde {sub R} parameter space where this is the case with particular emphasis on light sneutrinos with masses below 10 GeV. We discuss implications for direct and indirect dark matter searches, including the relevant uncertainties, as well as consequences for collider phenomenology.

  9. The C-4 Dark Matter Experiment

    SciTech Connect (OSTI)

    Bonicalzi, Ricco; Collar, J. I.; Colaresi, J.; Fast, James E.; Fields, N.; Fuller, Erin S.; Hai, M.; Hossbach, Todd W.; Kos, Marek S.; Orrell, John L.; Overman, Cory T.; Reid, Douglas J.; VanDevender, Brent A.; Wiseman, Clinton G.; Yocum, K. M.

    2013-06-01

    Abstract We describe the experimental design of C-4, an expansion of the CoGeNT dark matter search to four identical detectors each approximately three times the mass of the p-type point contact (PPC) germanium diode presently taking data at the Soudan Underground Laboratory. Expected reductions of radioactive backgrounds and energy threshold are discussed, including an estimate of the additional sensitivity to low-mass dark matter candidates to be obtained with this search.

  10. Ultrafast Spectroscopy of Warm Dense Matter

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Ultrafast Spectroscopy of Warm Dense Matter Print Being neither solid, liquid, gas, nor plasma, warm dense matter (WDM) occupies a no man's land in the map of material phases. Its temperature can range between that of planetary cores (tens of thousands K) to that of stellar cores (hundreds of thousands K). Not only is it prevalent throughout the universe, it is relevant to inertial confinement fusion (ICF) and material performance under extreme conditions. However, because of its extreme